text stringlengths 1 3.55k | source stringlengths 24 207 | emb listlengths 1.02k 1.02k |
|---|---|---|
and potential energy becomes mass in a system. why is it we don β t ordinarily notice this? in fact, conservation of mass ( meaning total mass is constant ) was one of the great laws verified by 19th - century science. why was it not noticed to be incorrect? the following example helps answer these questions. example 2... | openstax_college_physics_2e-web_7zesafu | [
-0.008864770643413067,
0.03330802544951439,
0.02019365504384041,
0.00892634317278862,
-0.035165801644325256,
-0.0007703525479882956,
0.019704923033714294,
-0.013145591132342815,
-0.006778258364647627,
0.06500163674354553,
0.0544174425303936,
-0.005243359599262476,
0.021721437573432922,
-0.... |
very small, since energy is divided by, a very large number. we would have to be able to measure the mass of the battery to a precision of a billionth of a percent, or 1 part in, to notice this increase. it is no wonder that the mass variation is not readily observed. in fact, this change in mass is so small that we ma... | openstax_college_physics_2e-web_7zesafu | [
-0.0038901290390640497,
0.008984189480543137,
0.013418537564575672,
0.018056634813547134,
-0.03318154439330101,
0.008475768379867077,
0.0038188782054930925,
-0.007619514130055904,
-0.017135556787252426,
0.04840574786067009,
0.07229156047105789,
0.0024577174335718155,
0.01941944845020771,
-... |
28. 6 β’ relativistic energy 1263 kinetic energy and the ultimate speed limit kinetic energy is energy of motion. classically, kinetic energy has the familiar expression. the relativistic expression for kinetic energy is obtained from the work - energy theorem. this theorem states that the net work on a system goes into... | openstax_college_physics_2e-web_7zesafu | [
-0.027828093618154526,
0.004581650253385305,
0.021755417808890343,
0.0318186953663826,
-0.012342618778347969,
-0.0006833794759586453,
0.0033966570626944304,
-0.022738514468073845,
-0.03742655739188194,
0.06859851628541946,
-0.0032255975529551506,
0.01941726915538311,
0.006334084086120129,
... |
mass. all of this is consistent with the fact that velocities less than always add to less than. both the relativistic form for kinetic energy and the ultimate speed limit being have been confirmed in detail in numerous experiments. no matter how much energy is put into 28. 50 28. 51 relativistic kinetic energy relativ... | openstax_college_physics_2e-web_7zesafu | [
-0.02057274430990219,
0.029207011684775352,
0.01615261659026146,
0.01796635240316391,
0.0059042335487902164,
0.0033086221665143967,
0.03205057978630066,
-0.009925154969096184,
-0.04395946487784386,
0.05905719846487045,
-0.0008933079661801457,
0.021370558068156242,
0.007002042140811682,
-0.... |
28. 56 the speed of light no object with mass can attain the speed of light. 1264 28 β’ special relativity access for free at openstax. org accelerating a mass, its velocity can only approach β not reach β the speed of light. figure 28. 22 this graph of versus velocity shows how kinetic energy approaches infinity as vel... | openstax_college_physics_2e-web_7zesafu | [
-0.012624537572264671,
-0.004336901940405369,
-0.010476771742105484,
0.018514763563871384,
0.007605810184031725,
0.011652698740363121,
-0.01301526464521885,
-0.0023950962349772453,
-0.014187288470566273,
0.06624940037727356,
-0.007064396515488625,
0.027751924470067024,
0.011577431112527847,
... |
28. 6 β’ relativistic energy 1265 solution for ( b ) 1. list the knowns. ; 2. list the unknown. 3. choose the appropriate equation. 4. plug the knowns into the equation. 5. convert units. discussion as might be expected, since the velocity is 99. 0 % of the speed of light, the classical kinetic energy is significantly o... | openstax_college_physics_2e-web_7zesafu | [
0.0022441500332206488,
0.002046599518507719,
-0.0030803896952420473,
0.012271285988390446,
-0.010563179850578308,
0.009335555136203766,
-0.004623077344149351,
-0.02732005901634693,
-0.02231723442673683,
0.04335547238588333,
0.008059117011725903,
0.005022508557885885,
0.011949791572988033,
... |
these particles and some of their characteristics will be covered in particle physics. figure 28. 23 the fermi national accelerator laboratory, near batavia, illinois, was a subatomic particle collider that accelerated protons and antiprotons to attain energies up to 1 tev ( a trillion electronvolts ). the circular pon... | openstax_college_physics_2e-web_7zesafu | [
-0.010332559235394001,
0.01909172162413597,
-0.017321893945336342,
-0.011997797526419163,
-0.015658626332879066,
0.017495734617114067,
-0.028596961870789528,
-0.04165074601769447,
-0.0068168179132044315,
0.04525453597307205,
0.007095745764672756,
0.029544541612267494,
0.016588231548666954,
... |
28. 61 1266 28 β’ special relativity access for free at openstax. org relativistically, we can obtain a relationship between energy and momentum by algebraically manipulating their definitions. this produces where is the relativistic total energy and is the relativistic momentum. this relationship between relativistic e... | openstax_college_physics_2e-web_7zesafu | [
-0.012165717780590057,
0.03835345804691315,
0.013847455382347107,
0.03439199551939964,
-0.006608078256249428,
0.012198232114315033,
-0.02176671102643013,
-0.0130697563290596,
-0.05115426704287529,
0.043664030730724335,
-0.01740284636616707,
0.010412194766104221,
-0.0003105906944256276,
-0.... |
28. 63 problem - solving strategies for relativity 1. examine the situation to determine that it is necessary to use relativity. relativistic effects are related to, the quantitative relativistic factor. if is very close to 1, then relativistic effects are small and differ very little from the usually easier classical ... | openstax_college_physics_2e-web_7zesafu | [
-0.002642484148964286,
0.019558405503630638,
0.001434204401448369,
0.007801388390362263,
-0.025084927678108215,
-0.0007015689043328166,
0.0024635049048811197,
0.00738224433735013,
-0.02108054794371128,
0.0650574341416359,
-0.010693161748349667,
-0.005191352684050798,
0.01246002409607172,
-... |
28. 64 1268 28 β’ special relativity access for free at openstax. org glossary classical velocity addition the method of adding velocities when ; velocities add like regular numbers in one - dimensional motion :, where is the velocity between two observers, is the velocity of an object relative to one observer, and is t... | openstax_college_physics_2e-web_7zesafu | [
-0.027387941256165504,
0.0320451520383358,
0.011042189784348011,
0.0037339453119784594,
-0.009888321161270142,
0.005903204437345266,
-0.007409394718706608,
-0.023417320102453232,
-0.011866740882396698,
0.07026414573192596,
0.013170410878956318,
0.00015608039393555373,
0.0031711668707430363,
... |
of an object moving at relativistic velocity ;, where is the rest mass of the object, is its velocity relative to an observer, and the relativistic factor relativistic velocity addition the method of adding velocities of an object moving at a relativistic speed :, where is the relative velocity between two observers, i... | openstax_college_physics_2e-web_7zesafu | [
-0.031871065497398376,
0.024809028953313828,
0.005641644354909658,
0.0066465833224356174,
-0.029568292200565338,
-0.0015816094819456339,
-0.014736580662429333,
-0.027040844783186913,
-0.01947650872170925,
0.06294883042573929,
-0.022162361070513725,
-0.011587055400013924,
0.014272268861532211... |
28. 1 einstein β s postulates β’ relativity is the study of how different observers measure the same event. β’ modern relativity is divided into two parts. special relativity deals with observers who are in uniform ( unaccelerated ) motion, whereas general relativity includes accelerated relative motion and gravity. mode... | openstax_college_physics_2e-web_7zesafu | [
-0.0029636856634169817,
0.0017478256486356258,
0.006334047764539719,
-0.026966819539666176,
-0.027879228815436363,
0.02233188785612583,
-0.007953372783958912,
-0.003917599096894264,
0.02485627308487892,
0.05975789949297905,
0.017607394605875015,
-0.018998339772224426,
0.007238681428134441,
... |
28. 2 simultaneity and time dilation β’ two events are defined to be simultaneous if an observer measures them as occurring at the same time. they are not necessarily simultaneous to all observers β simultaneity is not absolute. β’ time dilation is the phenomenon of time passing slower for an observer who is moving relat... | openstax_college_physics_2e-web_7zesafu | [
0.011589269153773785,
0.03048824891448021,
0.01384491566568613,
-0.004388183355331421,
0.002592712640762329,
0.01963799260556698,
-0.027376689016819,
-0.02051560766994953,
-0.024585789069533348,
0.08082989603281021,
0.001356244320049882,
-0.0062649729661643505,
-0.027816303074359894,
-0.04... |
28. 4 relativistic addition of velocities β’ with classical velocity addition, velocities add like regular numbers in one - dimensional motion :, where is the velocity between two observers, is the velocity of an object relative to one observer, and is the velocity relative to the other observer. β’ velocities cannot add... | openstax_college_physics_2e-web_7zesafu | [
-0.015452496707439423,
0.02241312898695469,
0.0009008870692923665,
-0.01654977723956108,
0.0010490755084902048,
-0.0012325262650847435,
-0.031732384115457535,
0.003726113820448518,
-0.008968979120254517,
0.09269401431083679,
-0.011327538639307022,
0.00400596484541893,
0.011777225881814957,
... |
28. 5 relativistic momentum β’ the law of conservation of momentum is valid whenever the net external force is zero and for relativistic momentum. relativistic momentum is classical momentum multiplied by the relativistic factor. β’, where is the rest mass of the object, is its velocity relative to an observer, and the r... | openstax_college_physics_2e-web_7zesafu | [
-0.01169627532362938,
0.007383317686617374,
0.007078414782881737,
0.012102698907256126,
-0.0005114084342494607,
-0.017221668735146523,
-0.003033638233318925,
-0.009214695543050766,
-0.01841103658080101,
0.07035648822784424,
-0.011949840001761913,
0.04444151744246483,
0.0071550398133695126,
... |
28. 6 relativistic energy β’ relativistic energy is conserved as long as we define it to include the possibility of mass changing to energy. β’ total energy is defined as :, where. β’ rest energy is, meaning that mass is a form of energy. if energy is stored in an object, its mass increases. mass can be destroyed to relea... | openstax_college_physics_2e-web_7zesafu | [
0.005616097245365381,
0.027103712782263756,
0.007621523924171925,
0.022868193686008453,
-0.017815349623560905,
0.007668484002351761,
-0.003056299639865756,
-0.012168383225798607,
-0.017506437376141548,
0.05992092192173004,
0.0002198192960349843,
0.012143316678702831,
0.006384487729519606,
... |
##sed time for a process seem to be longer, an observer moving relative to the process or an observer moving with the process? which observer measures proper time? 6. how could you travel far into the future without aging significantly? could this method also allow you to travel into the past? | openstax_college_physics_2e-web_7zesafu | [
0.05054677277803421,
0.004771786276251078,
0.007963169366121292,
0.019358081743121147,
-0.002605665009468794,
0.019271640107035637,
-0.03483961150050163,
-0.005071757826954126,
-0.018827620893716812,
0.068409264087677,
-0.012573927640914917,
-0.02042090706527233,
0.0404009185731411,
-0.038... |
28. 3 length contraction 7. to whom does an object seem greater in length, an observer moving with the object or an observer moving relative to the object? which observer measures the object β s proper length? 8. relativistic effects such as time dilation and length contraction are present for cars and airplanes. why d... | openstax_college_physics_2e-web_7zesafu | [
0.042869243770837784,
0.00999524537473917,
-0.0035462593659758568,
0.00025381759041920304,
0.014058645814657211,
0.02848788909614086,
-0.011059723794460297,
0.006766733713448048,
0.010003579780459404,
0.06805060058832169,
0.039479874074459076,
-0.006499872542917728,
-0.020908761769533157,
... |
28. 4 relativistic addition of velocities 10. explain the meaning of the terms β red shift β and β blue shift β as they relate to the relativistic doppler effect. 11. what happens to the relativistic doppler effect when relative velocity is zero? is this the expected result? 12. is the relativistic doppler effect consi... | openstax_college_physics_2e-web_7zesafu | [
0.012994225136935711,
0.01744736358523369,
-0.018666965886950493,
0.024433547630906105,
-0.0059687173925340176,
0.002187019446864724,
-0.035055287182331085,
0.007147616241127253,
-0.03031429648399353,
0.11013606935739517,
0.00838905107229948,
0.026855211704969406,
-0.007944663986563683,
-0... |
28. 6 relativistic energy 16. how are the classical laws of conservation of energy and conservation of mass modified by modern relativity? 17. what happens to the mass of water in a pot when it cools, assuming no molecules escape or are added? is this observable in practice? explain. 18. consider a thought experiment. ... | openstax_college_physics_2e-web_7zesafu | [
0.005007827188819647,
0.006401287391781807,
0.007771559990942478,
0.004900765139609575,
-0.023642295971512794,
0.016942046582698822,
-0.020888544619083405,
-0.001820851699449122,
0.011371210217475891,
0.07737543433904648,
0.021928995847702026,
0.011160043999552727,
0.029548540711402893,
-0... |
28. 2 simultaneity and time dilation 1. ( a ) what is if? ( b ) if? 2. ( a ) what is if? ( b ) if? 3. particles called - mesons are produced by accelerator beams. if these particles travel at and live when at rest relative to an observer, how long do they live as viewed in the laboratory? 4. suppose a particle called a... | openstax_college_physics_2e-web_7zesafu | [
0.021724356338381767,
-0.01277181413024664,
-0.012978562153875828,
-0.018773965537548065,
0.003996965941041708,
-0.006639862898737192,
-0.03880620375275612,
0.0007682494469918311,
-0.03228502720594406,
0.06374241411685944,
0.011403759941458702,
0.00328569277189672,
0.026997989043593407,
-0... |
28. 3 length contraction 12. a spaceship, 200 m long as seen on board, moves by the earth at. what is its length as measured by an earth - bound observer? 13. how fast would a 6. 0 m - long sports car have to be going past you in order for it to appear only 5. 5 m long? 1272 28 β’ problems & exercises access for free at... | openstax_college_physics_2e-web_7zesafu | [
0.0547233484685421,
0.004269808065146208,
-0.006882994435727596,
-0.01320780348032713,
-0.025121226906776428,
0.04527537524700165,
-0.0006599952466785908,
0.0278401430696249,
-0.015991687774658203,
0.05842209234833717,
0.08331408351659775,
0.014227028004825115,
-0.006243221927434206,
-0.03... |
28. 2 to travel 4. 30 ly at ( as measured by the earth - bound observer )? ( b ) how long does it take according to the astronaut? ( c ) verify that these two times are related through time dilation with as given. 17. ( a ) how fast would an athlete need to be running for a 100 - m race to look 100 yd long? ( b ) is th... | openstax_college_physics_2e-web_7zesafu | [
0.03289071470499039,
0.00795149989426136,
-0.002631027717143297,
-0.009447980672121048,
-0.03278797119855881,
0.02984391339123249,
0.0010187700390815735,
0.007325956132262945,
-0.038030605763196945,
0.06889072805643082,
0.029861774295568466,
-0.02386314421892166,
-0.004827909171581268,
-0.... |
28. 4 relativistic addition of velocities 20. suppose a spaceship heading straight towards the earth at can shoot a canister at relative to the ship. ( a ) what is the velocity of the canister relative to the earth, if it is shot directly at the earth? ( b ) if it is shot directly away from the earth? 21. repeat the pr... | openstax_college_physics_2e-web_7zesafu | [
0.026528730988502502,
0.038175031542778015,
0.0038720197044312954,
0.007148406933993101,
-0.04409738630056381,
-0.0006888043135404587,
-0.04961869493126869,
0.02564922906458378,
-0.025743918493390083,
0.0902777910232544,
-0.0062063466757535934,
0.008513882756233215,
-0.006736459210515022,
... |
when a missile is shot from one spaceship towards another, it leaves the first at and approaches the other at. what is the relative velocity of the two ships? 29. what is the relative velocity of two spaceships if one fires a missile at the other at and the other observes it to approach at? 30. near the center of our g... | openstax_college_physics_2e-web_7zesafu | [
0.03399233520030975,
0.06941349059343338,
0.0002507013559807092,
0.01654491201043129,
-0.03789099305868149,
-0.0007042131619527936,
-0.0362325944006443,
0.02595161646604538,
-0.011361204087734222,
0.07790117710828781,
-0.018415620550513268,
0.0166005976498127,
-0.011050081811845303,
-0.038... |
how long will it then take for a radio signal to be beamed back? ( all of this is possible in principle, but not practical. ) | openstax_college_physics_2e-web_7zesafu | [
-0.0018444155575707555,
0.011263435706496239,
-0.004417128395289183,
0.023302441462874413,
-0.00769340293481946,
0.0017478325171396136,
-0.019812867045402527,
0.004540813621133566,
0.015637071803212166,
0.07174620032310486,
0.023882951587438583,
0.008746305480599403,
-0.0018031173385679722,
... |
28. 5 relativistic momentum 35. find the momentum of a helium nucleus having a mass of that is moving at. 36. what is the momentum of an electron traveling at? 37. ( a ) find the momentum of a asteroid heading towards the earth at. ( b ) find the ratio of this momentum to the classical momentum. ( hint : use the approx... | openstax_college_physics_2e-web_7zesafu | [
0.029174400493502617,
0.043358638882637024,
0.008217689581215382,
-0.003024371573701501,
0.006893375422805548,
0.02425268292427063,
0.0075182621367275715,
0.008405569940805435,
-0.021319670602679253,
0.04584360867738724,
0.011290766298770905,
0.01731845736503601,
0.001160227693617344,
-0.0... |
28. 6 relativistic energy 43. what is the rest energy of an electron, given its mass is? give your answer in joules and mev. 44. find the rest energy in joules and mev of a proton, given its mass is. 45. if the rest energies of a proton and a neutron ( the two constituents of nuclei ) are 938. 3 and 939. 6 mev respecti... | openstax_college_physics_2e-web_7zesafu | [
0.005295404698699713,
0.007260623387992382,
0.009296869859099388,
0.00806589424610138,
-0.03547890484333038,
-0.018987921997904778,
0.007926286198198795,
-0.010676734149456024,
-0.031873688101768494,
0.04672360420227051,
0.012140878476202488,
0.004614836536347866,
0.020898303017020226,
-0.... |
. a muon has a rest mass energy of 105. 7 mev, and it decays into an electron and a massless particle. ( a ) if all the lost mass is converted into the electron β s kinetic energy, find for the electron. ( b ) what is the electron β s velocity? 52. a - meson is a particle that decays into a muon and a massless particle... | openstax_college_physics_2e-web_7zesafu | [
0.006647481583058834,
0.024747319519519806,
-0.015249251388013363,
0.03564375638961792,
-0.013083360157907009,
-0.004538675304502249,
-0.009170315228402615,
-0.012565855868160725,
-0.040424980223178864,
0.054387420415878296,
0.027435073629021645,
0.049866288900375366,
0.021415721625089645,
... |
##ilation. ( b ) if this energy is given to a proton in the form of kinetic energy, what is its velocity? ( c ) if this energy is given to another electron in the form of kinetic energy, what is its velocity? 57. what is the kinetic energy in mev of a - meson that lives as measured in the laboratory, and when at rest r... | openstax_college_physics_2e-web_7zesafu | [
0.03358003869652748,
0.01970987394452095,
-0.00008074477955233306,
0.019769303500652313,
-0.006404787302017212,
0.014646868221461773,
0.007028206717222929,
-0.005311277695000172,
-0.054319050163030624,
0.06319205462932587,
-0.005403938703238964,
0.03988607972860336,
0.0464898943901062,
-0.... |
938. 3 mev accelerated through an effective potential of 1. 0 tv ( teravolt ) at fermilab outside chicago? 62. ( a ) what is the effective accelerating potential for electrons at the stanford linear accelerator, if for them? ( b ) what is their total energy ( nearly the same as kinetic in this case ) in gev? 63. ( a ) ... | openstax_college_physics_2e-web_7zesafu | [
0.020422494038939476,
0.014815614558756351,
0.0027081952430307865,
0.04138081520795822,
-0.03668795898556709,
0.008034038357436657,
-0.013371169567108154,
0.0010032737627625465,
-0.03426282852888107,
0.04283710569143295,
0.03630797564983368,
0.023600835353136063,
0.016174348071217537,
-0.0... |
to be destroyed to get it into a low earth orbit, neglecting the decrease in gravity? ( assume an orbital altitude of 250 km, and calculate both the kinetic energy ( classical ) and the gravitational potential energy needed. ) ( b ) if the ship has a mass of ( 100 tons ), what total yield nuclear explosion in tons of t... | openstax_college_physics_2e-web_7zesafu | [
0.030359098687767982,
0.01841900497674942,
0.011923166923224926,
0.0210115909576416,
-0.042501091957092285,
-0.0027874945662915707,
0.000590248208027333,
0.021231060847640038,
-0.023052284494042397,
0.04352898150682449,
0.012711509130895138,
0.023218918591737747,
0.01899898238480091,
-0.05... |
50. 0 mev. ( a ) what is the proton β s kinetic energy? ( b ) what is unreasonable about this result? ( c ) which assumptions are unreasonable or inconsistent? 71. construct your own problem consider a highly relativistic particle. discuss what is meant by the term β highly relativistic. β ( note that, in part, it mean... | openstax_college_physics_2e-web_7zesafu | [
0.016594989225268364,
0.0013531070435419679,
0.01374075748026371,
0.031334809958934784,
-0.03588184714317322,
0.010071039199829102,
0.004679267760366201,
0.01410933118313551,
-0.04894080385565758,
0.0697561576962471,
0.05072738230228424,
0.005187470931559801,
0.026642881333827972,
-0.04999... |
β’ problems & exercises access for free at openstax. org introduction to quantum physics chapter 29 quantum physics 29. 1 quantization of energy 29. 2 the photoelectric effect 29. 3 photon energies and the electromagnetic spectrum 29. 4 photon momentum 29. 5 the particle - wave duality 29. 6 the wave nature of matter 29... | openstax_college_physics_2e-web_7zesafu | [
-0.0005178403807803988,
-0.002030747476965189,
0.05657905340194702,
-0.00015288559370674193,
-0.025098763406276703,
-0.004373722244054079,
-0.03537055850028992,
-0.02281157113611698,
-0.062211427837610245,
0.10431726276874542,
0.013321097008883953,
0.0062753427773714066,
0.02316981554031372,... |
29. 8 the particle - wave duality reviewed quantum mechanics is the branch of physics needed to deal with submicroscopic objects. because these objects are smaller than we can observe directly with our senses and generally must be observed with the aid of instruments, parts of quantum mechanics seem as foreign and biza... | openstax_college_physics_2e-web_7zesafu | [
0.007950162515044212,
-0.02546689473092556,
0.026054108515381813,
-0.015429976396262646,
-0.024720383808016777,
-0.007515345234423876,
0.009196838364005089,
-0.02744036354124546,
-0.042826373130083084,
0.07328000664710999,
0.051189254969358444,
-0.0027455012314021587,
0.0025708682369440794,
... |
certain discrete values and do not have every conceivable value. quantized is the opposite of continuous. we cannot have a fraction of an atom, or part of an electron β s charge, or 14 - 1 / 3 cents, for example. rather, everything is built of integral multiples of these substructures. quantum physics is the branch of ... | openstax_college_physics_2e-web_7zesafu | [
-0.022289564833045006,
-0.02571726217865944,
0.002115843119099736,
-0.017106609418988228,
-0.006875331979244947,
-0.01316640805453062,
0.017331140115857124,
-0.01637728326022625,
-0.08197463303804398,
0.05242394655942917,
0.05430918186903,
-0.003698950167745352,
0.0037406478077173233,
-0.0... |
29. 1 quantization of energy learning objectives by the end of this section, you will be able to : β’ explain max planck β s contribution to the development of quantum mechanics. β’ explain why atomic spectra indicate quantization. planck β s contribution energy is quantized in some systems, meaning that the system can h... | openstax_college_physics_2e-web_7zesafu | [
0.01326064858585596,
-0.006466645747423172,
0.04545111209154129,
0.026744825765490532,
0.00392976775765419,
0.012055003084242344,
0.004469114355742931,
-0.030744308605790138,
-0.0999821275472641,
0.05965228006243706,
0.01974651776254177,
-0.0022117176558822393,
0.02790250815451145,
-0.0177... |
thus, is jet black. ideal radiators are therefore called blackbodies, and their em radiation is called blackbody radiation. it was discussed that the total intensity of the radiation varies as the fourth power of the absolute temperature of the body, and that the peak of the spectrum shifts to shorter wavelengths at hi... | openstax_college_physics_2e-web_7zesafu | [
0.011566780507564545,
-0.009986273013055325,
0.04464181885123253,
0.01227074395865202,
-0.01621783711016178,
-0.014099002815783024,
-0.014825653284788132,
-0.001636219210922718,
-0.04994433373212814,
0.07025538384914398,
0.0316692590713501,
-0.027600422501564026,
0.05083558335900307,
-0.04... |
discrete stair steps rather than being able to move up and down a continuous slope. your potential energy takes on discrete values as you move from step to step. using the quantization of oscillators, planck was able to correctly describe the experimentally known shape of the blackbody spectrum. this was the first indi... | openstax_college_physics_2e-web_7zesafu | [
0.0054370202124118805,
-0.03038848005235195,
0.03362060338258743,
-0.005490164738148451,
-0.0334530733525753,
0.00951319094747305,
0.019146624952554703,
0.01903674751520157,
-0.005750957410782576,
0.06409183889627457,
0.02879098244011402,
-0.006610526237636805,
0.036985043436288834,
-0.010... |
29. 1 β’ quantization of energy 1279 its analysis is based on atoms and molecules. it was such a revolutionary departure from classical physics that planck himself was reluctant to accept his own idea that energy states are not continuous. the general acceptance of planck β s energy quantization was greatly enhanced by ... | openstax_college_physics_2e-web_7zesafu | [
-0.0014869363512843847,
-0.006199995521456003,
0.05397816002368927,
0.016407765448093414,
-0.037206318229436874,
0.03283952176570892,
-0.008366089314222336,
0.002895178273320198,
-0.06407902389764786,
0.03901471570134163,
0.008848218247294426,
-0.006997925229370594,
0.003942062612622976,
-... |
light. we also see examples in neon signs and candle flames. studies of emissions of hot gases began more than two centuries ago, and it was soon recognized that these emission spectra contained huge amounts of information. the type of gas and its temperature, for example, could be determined. we now know that these em... | openstax_college_physics_2e-web_7zesafu | [
0.011054323054850101,
-0.008177408017218113,
0.04385972023010254,
0.011847874149680138,
-0.031821511685848236,
0.003199795726686716,
-0.03794308006763458,
-0.02192770503461361,
0.010852234438061714,
0.06395324319601059,
0.027543291449546814,
-0.032518260180950165,
0.031643129885196686,
-0.... |
atoms without looking at them? try out different models by shooting light at the atom. check how the prediction of the model matches the experimental results. click to view content ( https : / / openstax. org / l / 28atom _ model ). | openstax_college_physics_2e-web_7zesafu | [
0.005285185296088457,
-0.037671830505132675,
-0.014955571852624416,
-0.020912213250994682,
-0.017403049394488335,
-0.015507500618696213,
-0.03320072218775749,
0.01449541188776493,
0.016247563064098358,
0.07917460054159164,
0.040637701749801636,
-0.01573096215724945,
0.03350413590669632,
-0... |
29. 2 the photoelectric effect learning objectives by the end of this section, you will be able to : β’ describe a typical photoelectric - effect experiment. β’ determine the maximum kinetic energy of photoelectrons ejected by photons of one energy or wavelength, when given the maximum kinetic energy of photoelectrons fo... | openstax_college_physics_2e-web_7zesafu | [
-0.03429543599486351,
0.0185785461217165,
0.025421814993023872,
0.03986093029379845,
-0.05184998735785484,
-0.014527936466038227,
-0.06506428122520447,
0.004607838578522205,
0.0157676599919796,
0.053747743368148804,
-0.012165012769401073,
-0.010611054487526417,
0.04136668145656586,
-0.0347... |
will be collected on the wire. since the electron energy in ev is, where is the electron charge and is the potential difference, the electron energy can be measured by adjusting the retarding voltage between the wire and the plate. the voltage that stops the electrons from reaching the wire equals the energy in ev. for... | openstax_college_physics_2e-web_7zesafu | [
-0.02147863805294037,
0.043601829558610916,
-0.02245626412332058,
0.019136885181069374,
-0.046313755214214325,
-0.042834509164094925,
0.009440720081329346,
-0.023368628695607185,
-0.01825093664228916,
0.035523563623428345,
-0.0034274067729711533,
0.021963194012641907,
0.049723248928785324,
... |
3. 00 ev. the number of electrons ejected can be determined by measuring the current between the wire and plate. the more light, the more electrons ; a little circuitry allows this device to be used as a light meter. what is really important about the photoelectric effect is what albert einstein deduced from it. einste... | openstax_college_physics_2e-web_7zesafu | [
-0.006854556966573,
-0.0064158206805586815,
0.02068699151277542,
0.008587016724050045,
-0.02690514177083969,
-0.010359846986830235,
-0.03708793595433235,
-0.006182549521327019,
-0.012823008932173252,
0.03834575414657593,
0.03037169761955738,
-0.024940449744462967,
0.030620353296399117,
-0.... |
29. 2 β’ the photoelectric effect 1281 photon energy is where is the energy of a photon of frequency and is planck β s constant. this revolutionary idea looks similar to planck β s quantization of energy states in blackbody oscillators, but it is quite different. it is the quantization of em radiation itself. em waves a... | openstax_college_physics_2e-web_7zesafu | [
0.004645795561373234,
-0.01643352210521698,
0.0214229803532362,
0.006010038778185844,
-0.022354358807206154,
-0.007002527825534344,
-0.05613046512007713,
-0.012975617311894894,
-0.0523499920964241,
0.07196538150310516,
-0.013174375519156456,
-0.01729934848845005,
0.038067370653152466,
-0.0... |
in which all photons have the same energy. 1. if we vary the frequency of the em radiation falling on a material, we find the following : for a given material, there is a threshold frequency for the em radiation below which no electrons are ejected, regardless of intensity. individual photons interact with individual e... | openstax_college_physics_2e-web_7zesafu | [
-0.014270605519413948,
0.03644714877009392,
-0.009647020138800144,
0.009788553230464458,
0.002614861587062478,
-0.02828250639140606,
-0.051106683909893036,
0.0027781357057392597,
-0.042146947234869,
0.050847020000219345,
-0.011396468617022038,
0.01199138443917036,
0.03067566268146038,
-0.0... |
partly used to break the electron away from the material. the remainder goes into the ejected electron β s kinetic energy. in equation form, this is given by where is the maximum kinetic energy of the ejected electron, is the photon β s energy, and be is the binding energy of the electron to the particular material. ( ... | openstax_college_physics_2e-web_7zesafu | [
-0.009409279562532902,
-0.005119435489177704,
0.012166243977844715,
0.03770966827869415,
-0.014629382640123367,
-0.045464351773262024,
-0.03655833750963211,
0.013873111456632614,
-0.015851030126214027,
0.022571062669157982,
-0.004658993799239397,
0.0368330255150795,
0.03673327714204788,
-0... |
29. 5 1282 29 β’ quantum physics access for free at openstax. org material. ) this equation, due to einstein in 1905, explains the properties of the photoelectric effect quantitatively. an individual photon of em radiation ( it does not come any other way ) interacts with an individual electron, supplying enough energy,... | openstax_college_physics_2e-web_7zesafu | [
-0.01056698989123106,
0.014681680127978325,
0.029122354462742805,
0.03323742002248764,
-0.020796531811356544,
-0.013477230444550514,
-0.042807064950466156,
0.002297046361491084,
-0.049955300986766815,
0.055727653205394745,
-0.024814140051603317,
-0.016671238467097282,
0.008213275112211704,
... |
. although his other contributions to theoretical physics were also noted in that award, special and general relativity were not fully recognized in spite of having been partially verified by experiment by 1921. although hero - worshipped, this great man never received nobel recognition for his most famous work β relat... | openstax_college_physics_2e-web_7zesafu | [
-0.014980394393205643,
-0.033587533980607986,
0.04102574288845062,
0.03768397122621536,
-0.05356406420469284,
-0.022701065987348557,
-0.04784069210290909,
0.02402820996940136,
-0.025190170854330063,
0.03969167545437813,
-0.004750070162117481,
-0.017608705908060074,
0.035576481372117996,
-0... |
29. 2 β’ the photoelectric effect 1283 combining these two equations gives the useful relationship now substituting known values yields converting to ev, the energy of the photon is solution for ( b ) finding the kinetic energy of the ejected electron is now a simple application of the equation. substituting the photon ... | openstax_college_physics_2e-web_7zesafu | [
-0.022952957078814507,
-0.00718919700011611,
0.015308406203985214,
0.01762683503329754,
-0.04827673360705376,
-0.019255956634879112,
-0.03571876138448715,
0.009390344843268394,
-0.017401302233338356,
0.08024605363607407,
-0.0077682496048510075,
-0.034708037972450256,
0.016870928928256035,
... |
click to view content ( https : / / openstax. org / l / 28photoelectric ). 29. 3 photon energies and the electromagnetic spectrum learning objectives by the end of this section, you will be able to : β’ explain the relationship between the energy of a photon in joules or electron volts and its wavelength or frequency. β’... | openstax_college_physics_2e-web_7zesafu | [
0.014195985160768032,
-0.004744839388877153,
-0.003108093049377203,
0.008300905115902424,
-0.03497576713562012,
-0.009910587221384048,
-0.035104840993881226,
-0.031089914962649345,
-0.05087236687541008,
0.037492044270038605,
-0.00816196296364069,
0.0022173658944666386,
0.033330287784338,
-... |
29. 11 1284 29 β’ quantum physics access for free at openstax. org ionizing radiation a photon is a quantum of em radiation. its energy is given by and is related to the frequency and wavelength of the radiation by where is the energy of a single photon and is the speed of light. when working with small systems, energy ... | openstax_college_physics_2e-web_7zesafu | [
0.0031791995279490948,
-0.007974201813340187,
0.011745262891054153,
-0.01533674355596304,
-0.0206083245575428,
-0.006366841960698366,
-0.03287076950073242,
-0.035703253000974655,
-0.06273926794528961,
0.06796462833881378,
0.026658864691853523,
-0.023172369226813316,
0.024897849187254906,
-... |
29. 3 β’ photon energies and the electromagnetic spectrum 1285 photons act as individual quanta and interact with individual electrons, atoms, molecules, and so on. the energy a photon carries is, thus, crucial to the effects it has. table 29. 1 lists representative submicroscopic energies in ev. when we compare photon ... | openstax_college_physics_2e-web_7zesafu | [
0.01951051875948906,
0.0047903358936309814,
0.030548935756087303,
0.015741316601634026,
-0.0317399688065052,
-0.024367183446884155,
-0.027946192771196365,
-0.008116294629871845,
-0.05553367733955383,
0.06834087520837784,
0.006127454806119204,
-0.009787916205823421,
0.04141736775636673,
-0.... |
as you can see in figure 29. 9, overlap with the low - frequency end of the ray range. since x rays have energies of kev and up, individual x - ray photons also can produce large amounts of ionization. at lower photon energies, x rays are not as penetrating as rays and are slightly less hazardous. x rays are ideal for ... | openstax_college_physics_2e-web_7zesafu | [
-0.013509939424693584,
0.01170174777507782,
0.04091372340917587,
0.008721471764147282,
-0.0021982097532600164,
-0.012939617969095707,
-0.04571957513689995,
0.0003686783602461219,
-0.032455578446388245,
0.04522423446178436,
0.0007972700987011194,
-0.024788161739706993,
0.05431843549013138,
... |
the cathode, so such a tube is called a cathode ray tube ( crt ), and various versions of them are found in older tv and computer screens as well as in x - ray machines. example 29. 2 x - ray photon energy and x - ray tube voltage find the maximum energy in ev of an x - ray photon produced by electrons accelerated thro... | openstax_college_physics_2e-web_7zesafu | [
-0.019443128257989883,
-0.020649131387472153,
0.018496016040444374,
0.037605077028274536,
-0.008118914440274239,
-0.04064751788973808,
-0.03282622992992401,
-0.011804484762251377,
-0.020418863743543625,
0.056290917098522186,
-0.004490422550588846,
0.0030811973847448826,
0.03752243146300316,
... |
29. 3 β’ photon energies and the electromagnetic spectrum 1287 discussion this example produces a result that can be applied to many similar situations. if you accelerate a single elementary charge, like that of an electron, through a potential given in volts, then its energy in ev has the same numerical value. thus a 5... | openstax_college_physics_2e-web_7zesafu | [
-0.007791984360665083,
0.0010942257940769196,
0.04157395660877228,
0.0068554445169866085,
-0.032521337270736694,
-0.005644260440021753,
-0.037897951900959015,
-0.012455218471586704,
-0.06232811138033867,
0.06765847653150558,
0.0057135275565087795,
-0.0017339957412332296,
0.049850188195705414... |
300 ev ) overlaps with the low end of the energy range of x rays, but uv is typically lower in energy. uv comes from the de - excitation of atoms that may be part of a hot solid or gas. these atoms can be given energy that they later release as uv by numerous processes, including electric discharge, nuclear explosion, ... | openstax_college_physics_2e-web_7zesafu | [
-0.02386537194252014,
-0.0004044749366585165,
0.03732360899448395,
0.0008032572804950178,
-0.039978496730327606,
-0.008322389796376228,
-0.05188349261879921,
-0.02193560265004635,
-0.04192463308572769,
0.05604400485754013,
0.007615343667566776,
0.0013780515873804688,
0.047411780804395676,
... |
29. 16 1288 29 β’ quantum physics access for free at openstax. org example 29. 3 photon energy and effects for uv short - wavelength uv is sometimes called vacuum uv, because it is strongly absorbed by air and must be studied in a vacuum. calculate the photon energy in ev for 100 - nm vacuum uv, and estimate the number ... | openstax_college_physics_2e-web_7zesafu | [
-0.011116307228803635,
-0.007842986844480038,
0.0326644666492939,
0.03299242630600929,
-0.029217058792710304,
-0.03373560309410095,
-0.023467568680644035,
-0.011813432909548283,
-0.026917628943920135,
0.08139625191688538,
0.01366947777569294,
0.0015862531727179885,
0.029909921810030937,
-0... |
for example, if a red photon of frequency encounters a molecule that has an energy step, equal to then the photon can be absorbed. violet flowers absorb red and reflect violet ; this implies there is no energy step between levels in the receptor molecule equal to the violet photon β s energy, but there is an energy ste... | openstax_college_physics_2e-web_7zesafu | [
-0.030546903610229492,
-0.01335085928440094,
0.02784932404756546,
0.01565360091626644,
-0.0490412637591362,
-0.030621754005551338,
-0.04013481363654137,
0.015161024406552315,
-0.013175706379115582,
0.08778925240039825,
-0.014279551804065704,
-0.006671990733593702,
0.037924278527498245,
-0.... |
29. 3 β’ photon energies and the electromagnetic spectrum 1289 figure 29. 13 why do the reds, yellows, and greens fade before the blues and violets when exposed to the sun, as with this poster? the answer is related to photon energy. ( credit : deb collins, flickr ) transparent materials, such as some glasses, do not ab... | openstax_college_physics_2e-web_7zesafu | [
-0.026160240173339844,
0.006167317274957895,
-0.008278434164822102,
0.01245186384767294,
-0.04056711867451668,
-0.015276387333869934,
-0.03430722653865814,
-0.003984314855188131,
0.0020420162472873926,
0.08172880113124847,
-0.008687232621014118,
-0.005958589259535074,
0.05382524058222771,
... |
29. 21 1290 29 β’ quantum physics access for free at openstax. org discussion this incredible number of photons per second is verification that individual photons are insignificant in ordinary human experience. it is also a verification of the correspondence principle β on the macroscopic scale, quantization becomes ess... | openstax_college_physics_2e-web_7zesafu | [
-0.021566743031144142,
-0.008241371251642704,
0.015429225750267506,
0.03471119701862335,
-0.050593052059412,
-0.01055159792304039,
-0.030395058915019035,
-0.008564733900129795,
-0.0324099026620388,
0.06694117933511734,
0.020409436896443367,
-0.029246563091874123,
0.017783358693122864,
-0.0... |
##s and do not ordinarily have the hazards of higher frequencies. when visible, ir, or microwave radiation is hazardous, such as the inducement of cataracts by microwaves, the hazard is due to huge numbers of photons acting together ( not to an accumulation of photons, such as sterilization by weak uv ). the negative e... | openstax_college_physics_2e-web_7zesafu | [
-0.036511510610580444,
0.01707596890628338,
-0.0029811400454491377,
0.019092287868261337,
-0.029616622254252434,
-0.02842966467142105,
-0.047711774706840515,
0.001144405105151236,
-0.021349966526031494,
0.07492752373218536,
0.022141948342323303,
-0.0013889055699110031,
0.03988098353147507,
... |
and additional studies since that time show no consistent, significant link between cancer and power - line fields. 29. 3 β’ photon energies and the electromagnetic spectrum 1291 electromagnetic - spectrum ) | openstax_college_physics_2e-web_7zesafu | [
-0.01305972971022129,
-0.0026589175686240196,
-0.0024212694261223078,
0.010751968249678612,
-0.007967643439769745,
-0.016283294185996056,
-0.009309567511081696,
-0.025269005447626114,
0.019821060821413994,
0.049865759909152985,
0.030594712123274803,
-0.0041579194366931915,
0.0464785508811473... |
29. 4 photon momentum learning objectives by the end of this section, you will be able to : β’ relate the linear momentum of a photon to its energy or wavelength, and apply linear momentum conservation to simple processes involving the emission, absorption, or reflection of photons. β’ account qualitatively for the incre... | openstax_college_physics_2e-web_7zesafu | [
0.040666207671165466,
-0.0008997063268907368,
0.007356820162385702,
-0.013741814531385899,
-0.003987335599958897,
0.027234405279159546,
-0.04422491416335106,
-0.0062100766226649284,
-0.03815244510769844,
0.0579635314643383,
-0.015869928523898125,
0.0327267050743103,
0.02566603757441044,
-0... |
29. 14 shows macroscopic evidence of photon momentum. figure 29. 14 the tails of the hale - bopp comet point away from the sun, evidence that light has momentum. dust emanating from the body of the comet forms this tail. particles of dust are pushed away from the sun by light reflecting from them. the blue ionized gas ... | openstax_college_physics_2e-web_7zesafu | [
0.032217301428318024,
0.010780255310237408,
0.023768791928887367,
-0.001155483303591609,
0.00021876837126910686,
0.0028940197080373764,
-0.04085008427500725,
0.005758446641266346,
0.0039619156159460545,
0.05586514249444008,
-0.011461404152214527,
-0.014930788427591324,
0.032579369843006134,
... |
are conserved in the collision. ( see figure 29. 15 ) he won a nobel prize in 1929 for the discovery of this scattering, now called the compton effect, because it helped prove that photon momentum is given by where is planck β s constant and is the photon wavelength. ( note that relativistic momentum given as is valid ... | openstax_college_physics_2e-web_7zesafu | [
0.01178903877735138,
-0.018634846433997154,
0.03453923016786575,
0.00589203042909503,
-0.012647474184632301,
-0.009145284071564674,
-0.025182457640767097,
-0.0032776615116745234,
-0.04405111446976662,
0.07203957438468933,
0.003236029762774706,
0.010891749523580074,
0.06064404919743538,
-0.... |
29. 4 β’ photon momentum 1293 strategy finding the photon momentum is a straightforward application of its definition :. if we find the photon momentum is small, then we can assume that an electron with the same momentum will be nonrelativistic, making it easy to find its velocity and kinetic energy from the classical f... | openstax_college_physics_2e-web_7zesafu | [
0.014208831824362278,
0.014637771993875504,
0.008067550137639046,
0.01659330353140831,
-0.007834186777472496,
-0.0002935367519967258,
-0.027325984090566635,
0.023609284311532974,
-0.04360516741871834,
0.04608391225337982,
-0.011077623814344406,
-0.004213552922010422,
-0.0011524094734340906,
... |
29. 26 29. 27 29. 28 | openstax_college_physics_2e-web_7zesafu | [
0.024075185880064964,
0.016999032348394394,
-0.02642769366502762,
0.010120549239218235,
-0.04535025730729103,
-0.001317297457717359,
0.024365602061152458,
0.016531305387616158,
-0.005782317370176315,
0.05678901821374893,
0.020714471116662025,
0.014375647529959679,
-0.007354251109063625,
-0... |
29. 29 1294 29 β’ quantum physics access for free at openstax. org figure 29. 16 ( a ) space sails have been proposed that use the momentum of sunlight reflecting from gigantic low - mass sails to propel spacecraft about the solar system. a russian test model of this ( the cosmos 1 ) was launched in 2005, but did not ma... | openstax_college_physics_2e-web_7zesafu | [
0.016362948343157768,
0.0009723493130877614,
0.0073517123237252235,
0.02126833237707615,
-0.007338910363614559,
0.027573654428124428,
-0.03214774280786514,
0.0033085797913372517,
-0.03574913740158081,
0.05737582966685295,
0.0023058862425386906,
-0.010524744167923927,
0.018726631999015808,
... |
image we detect. these detectors are used in biomedical imaging systems, and there is ongoing research into improving the efficiency of receiving photons, particularly by cooling detection systems and reducing thermal effects. 29. 4 β’ photon momentum 1295 discussion this value for momentum is the same as found before (... | openstax_college_physics_2e-web_7zesafu | [
-0.014713570475578308,
-0.001818851102143526,
0.0026081129908561707,
0.009392928332090378,
-0.02510419674217701,
0.02197558432817459,
-0.01605137065052986,
-0.01447925716638565,
-0.03105536848306656,
0.06868565082550049,
-0.004800091963261366,
0.002794805448502302,
0.03197517246007919,
-0.... |
29. 5 the particle - wave duality learning objectives by the end of this section, you will be able to : β’ explain what the term particle - wave duality means, and why it is applied to em radiation. we have long known that em radiation is a wave, capable of interference and diffraction. we now see that light can be mode... | openstax_college_physics_2e-web_7zesafu | [
-0.003172313328832388,
-0.016618788242340088,
-0.00015677315241191536,
-0.019413307309150696,
-0.03199199214577675,
0.008453166112303734,
-0.020262785255908966,
-0.022146807983517647,
-0.042142897844314575,
0.09555496275424957,
0.055743951350450516,
0.01214203517884016,
0.03630635514855385,
... |
strange, it is because we do not ordinarily observe details on the quantum level directly, and our observations yield either particle or wavelike properties, but never both simultaneously. | openstax_college_physics_2e-web_7zesafu | [
-0.03414278104901314,
-0.04467744380235672,
-0.014634665101766586,
-0.01409428846091032,
-0.01815028116106987,
-0.02534608542919159,
-0.024491621181368828,
0.017328361049294472,
-0.02829633466899395,
0.04061506688594818,
0.06198650598526001,
-0.049444619566202164,
0.0319194495677948,
-0.01... |
29. 33 problem - solving suggestion note that the forms of the constants and may be particularly useful for this section β s problems and exercises. 1296 29 β’ quantum physics access for free at openstax. org since we have a particle - wave duality for photons, and since we have seen connections between photons and matt... | openstax_college_physics_2e-web_7zesafu | [
-0.007109468802809715,
-0.00956820510327816,
0.017410092055797577,
-0.02438114583492279,
-0.019318219274282455,
0.008819297887384892,
-0.041777946054935455,
-0.02527812495827675,
-0.05504162609577179,
0.08696356415748596,
0.040102314203977585,
0.00748917181044817,
0.051074616611003876,
-0.... |
29. 6 the wave nature of matter learning objectives by the end of this section, you will be able to : β’ describe the davisson - germer experiment, and explain how it provides evidence for the wave nature of electrons. de broglie wavelength in 1923 a french physics graduate student named prince louis - victor de broglie... | openstax_college_physics_2e-web_7zesafu | [
0.005826413631439209,
0.014960070140659809,
0.0538153313100338,
-0.015982935205101967,
-0.035084210336208344,
0.04926569387316704,
-0.008549571968615055,
0.0035526095889508724,
-0.04082237184047699,
0.06033863499760628,
0.04004421830177307,
-0.0021889221388846636,
0.011258656159043312,
-0.... |
see its wave characteristics, the bowling ball would have to interact with something about in size β far smaller than anything known. when waves interact with objects much larger than their wavelength, they show negligible interference effects and move in straight lines ( such as light rays in geometric optics ). to ge... | openstax_college_physics_2e-web_7zesafu | [
-0.014782180078327656,
0.0019800541922450066,
0.051827337592840195,
-0.015106367878615856,
-0.030819587409496307,
0.03249581903219223,
-0.01756415143609047,
-0.0009030684013850987,
0.007485684938728809,
0.03710125386714935,
0.03521329164505005,
-0.017519788816571236,
0.028933851048350334,
... |
29. 6 β’ the wave nature of matter 1297 wavelength and are somewhat analogous to light interacting with a diffraction grating. ( see figure 29. 18. ) de broglie β s proposal of a wave nature for all particles initiated a remarkably productive era in which the foundations for quantum mechanics were laid. in 1926, the aus... | openstax_college_physics_2e-web_7zesafu | [
-0.007479528430849314,
-0.007765128742903471,
0.054479170590639114,
-0.03517652675509453,
-0.032390255481004715,
0.03548053279519081,
-0.0011256064753979445,
-0.010430550202727318,
-0.040130265057086945,
0.051047828048467636,
0.03814642131328583,
-0.013300569728016853,
0.023404529318213463,
... |
, once is obtained ( and it has been verified that is nonrelativistic ), the classical kinetic energy is simply solution for ( a ) substituting the nonrelativistic formula for momentum ( ) into the de broglie wavelength gives connections : waves all microscopic particles, whether massless, like photons, or having mass,... | openstax_college_physics_2e-web_7zesafu | [
0.001361403614282608,
0.012857100926339626,
0.01887451484799385,
-0.02108565717935562,
-0.004284261260181665,
0.019887039437890053,
0.0034263022243976593,
0.0017349006375297904,
-0.042631156742572784,
0.06127071753144264,
0.015970967710018158,
-0.03450024127960205,
0.010505431331694126,
-0... |
optical microscopes. ( see figure 29. 19. ) there are basically two types of electron microscopes. the transmission electron microscope ( tem ) accelerates electrons that are emitted from a hot filament ( the cathode ). the beam is broadened and then passes through the sample. a magnetic lens focuses the beam image ont... | openstax_college_physics_2e-web_7zesafu | [
0.019496887922286987,
-0.007034495007246733,
0.02378968708217144,
-0.012545113451778889,
0.0002744715893641114,
0.05722527951002121,
-0.042388953268527985,
-0.010949378833174706,
0.0058519537560641766,
0.026413319632411003,
0.014001780189573765,
-0.02620537579059601,
0.039025068283081055,
... |
29. 6 β’ the wave nature of matter 1299 figure 29. 19 schematic of a scanning electron microscope ( sem ) ( a ) used to observe small details, such as those seen in this image of a tooth of a himipristis, a type of shark ( b ). ( credit : dallas krentzel, flickr ) electrons were the first particles with mass to be direc... | openstax_college_physics_2e-web_7zesafu | [
0.00467910710722208,
-0.006421479396522045,
0.05540928244590759,
-0.026116708293557167,
-0.03566664457321167,
0.04297305643558502,
0.002234415616840124,
-0.017882226034998894,
-0.01962827518582344,
0.06668450683355331,
0.037163183093070984,
-0.036098968237638474,
0.018919361755251884,
0.00... |
electron wavelength, they show the same types of interference patterns as light does for diffraction gratings, as shown at top left in figure 29. 20. atoms are spaced at regular intervals in a crystal as parallel planes, as shown in the bottom part of figure 29. 20. the spacings between these planes act like the openin... | openstax_college_physics_2e-web_7zesafu | [
-0.02722501941025257,
-0.016767919063568115,
0.02143091708421707,
-0.0033582106698304415,
-0.025688394904136658,
-0.0067897336557507515,
-0.008163085207343102,
-0.03142816200852394,
-0.036744460463523865,
0.09963066130876541,
0.04392198845744133,
0.035926610231399536,
0.044047754257917404,
... |
29. 7 probability : the heisenberg uncertainty principle learning objectives by the end of this section, you will be able to : β’ use both versions of heisenberg β s uncertainty principle in calculations. β’ explain the implications of heisenberg β s uncertainty principle for measurements. probability distribution matter... | openstax_college_physics_2e-web_7zesafu | [
0.004588318057358265,
0.0019233264029026031,
0.02479616180062294,
-0.017645174637436867,
-0.015684718266129494,
0.00029051530873402953,
0.003637555055320263,
-0.027773559093475342,
-0.040325842797756195,
0.08717340975999832,
0.054437391459941864,
-0.020029954612255096,
0.03649183735251427,
... |
29. 7 β’ probability : the heisenberg uncertainty principle 1301 figure 29. 21 the building up of the diffraction pattern of electrons scattered from a crystal surface. each electron arrives at a definite location, which cannot be precisely predicted. the overall distribution shown at the bottom can be predicted as the ... | openstax_college_physics_2e-web_7zesafu | [
0.0015405267477035522,
-0.0014756082091480494,
0.017196668311953545,
-0.01648925058543682,
-0.016233209520578384,
-0.0027345633134245872,
-0.015992261469364166,
-0.013212957419455051,
-0.04069511964917183,
0.10810765624046326,
0.0550743043422699,
-0.013857964426279068,
0.030393967404961586,
... |
the detector. this can be observed for photons or electrons β for now, let us concentrate on electrons. you might imagine that the electrons are interfering with one another as any waves do. to test this, you can lower the intensity until there is never more than one electron between the slits and the screen. the same ... | openstax_college_physics_2e-web_7zesafu | [
-0.005781110841780901,
-0.007790743838995695,
-0.020911745727062225,
-0.0007659250986762345,
-0.028194308280944824,
0.0035125662107020617,
-0.041751664131879807,
-0.0007447237730957568,
-0.021004758775234222,
0.09401772171258926,
0.041106030344963074,
-0.0021225428208708763,
0.04283376410603... |
limit to absolute knowledge, even in principle. figure 29. 23 werner heisenberg was one of the best of those physicists who developed early quantum mechanics. not only did his work enable a description of nature on the very small scale, it also changed our view of the availability of knowledge. although he is universal... | openstax_college_physics_2e-web_7zesafu | [
0.02419220842421055,
0.0012600874761119485,
0.028951000422239304,
-0.004446817096322775,
-0.012143557891249657,
0.012218054383993149,
-0.014859647490084171,
-0.0051467628218233585,
-0.03021460399031639,
0.039060164242982864,
0.06539350003004074,
-0.03571417182683945,
0.035608116537332535,
... |
29. 7 β’ probability : the heisenberg uncertainty principle 1303 the uncertainty in position can be reduced by using a shorter - wavelength electron, since. but shortening the wavelength increases the uncertainty in momentum, since. conversely, the uncertainty in momentum can be reduced by using a longer - wavelength el... | openstax_college_physics_2e-web_7zesafu | [
0.023038320243358612,
0.013472480699419975,
0.043837983161211014,
-0.004711151123046875,
-0.020732881501317024,
0.0032713657710701227,
0.008055339567363262,
-0.02280634641647339,
-0.059377431869506836,
0.07829442620277405,
0.05871891602873802,
-0.04711532965302467,
0.022911014035344124,
0.... |
position of an electron in an atom is measured to an accuracy of 0. 0100 nm, what is the electron β s uncertainty in velocity? ( b ) if the electron has this velocity, what is its kinetic energy in ev? strategy the uncertainty in position is the accuracy of the measurement, or. thus the smallest uncertainty in momentum... | openstax_college_physics_2e-web_7zesafu | [
0.010889625176787376,
0.01621142402291298,
0.009194280952215195,
0.012348702177405357,
-0.008538399823009968,
-0.0102184247225523,
0.0372944176197052,
-0.02526410110294819,
-0.034172993153333664,
0.026907626539468765,
0.04839469864964485,
-0.013507314957678318,
0.016794411465525627,
-0.023... |
29. 47 1304 29 β’ quantum physics access for free at openstax. org solution for ( b ) although large, this velocity is not highly relativistic, and so the electron β s kinetic energy is discussion since atoms are roughly 0. 1 nm in size, knowing the position of an electron to 0. 0100 nm localizes it reasonably well insi... | openstax_college_physics_2e-web_7zesafu | [
0.014363488182425499,
0.011630022898316383,
0.04616404324769974,
0.024385828524827957,
-0.019215518608689308,
0.021106204017996788,
0.009949610568583012,
0.0010862413328140974,
-0.04987647011876106,
0.042829036712646484,
0.03821820393204689,
-0.02355881966650486,
0.023844445124268532,
-0.0... |
not possible to measure energy precisely β there will be an uncertainty in the measurement. in order to measure energy more precisely ( to make smaller ), we must increase. this time interval may be the amount of time we take to make the measurement, or it could be the amount of time a particular state exists, as in th... | openstax_college_physics_2e-web_7zesafu | [
0.02473408728837967,
0.014984510838985443,
0.015141252428293228,
-0.0017596455290913582,
-0.010165142826735973,
-0.018163194879889488,
0.011187952011823654,
-0.024377338588237762,
-0.01841447874903679,
0.04683753103017807,
0.05272361636161804,
-0.037685658782720566,
0.05882135033607483,
-0... |
29. 7 β’ probability : the heisenberg uncertainty principle 1305 now converting to ev yields discussion the lifetime of is typical of excited states in atoms β on human time scales, they quickly emit their stored energy. an uncertainty in energy of only a few millionths of an ev results. this uncertainty is small compar... | openstax_college_physics_2e-web_7zesafu | [
0.009695024229586124,
0.0321071483194828,
0.0279557928442955,
-0.0011491146869957447,
-0.025013595819473267,
0.014256688766181469,
0.003820381360128522,
-0.02836601249873638,
-0.02603229694068432,
0.05921105667948723,
0.05971282348036766,
-0.03490879759192467,
0.027140479534864426,
-0.0042... |
##ocuous enough, we shall see in later chapters that it allows the temporary creation of matter from nothing and has implications for how nature transmits forces over very small distances. finally, note that in the discussion of particles and waves, we have stated that individual measurements produce precise or particl... | openstax_college_physics_2e-web_7zesafu | [
-0.008785046637058258,
0.0031838370487093925,
0.015391450375318527,
-0.014213464222848415,
-0.0360034704208374,
0.01957252062857151,
-0.028659500181674957,
-0.0013847114751115441,
-0.04222388193011284,
0.06332097947597504,
0.04776562750339508,
-0.010774289257824421,
0.024860065430402756,
-... |
29. 51 1306 29 β’ quantum physics access for free at openstax. org figure 29. 24 on a quantum - mechanical scale ( i. e., very small ), particles with and without mass have wave properties. for example, both electrons and photons have wavelengths but also behave as particles. there are many submicroscopic particles in n... | openstax_college_physics_2e-web_7zesafu | [
-0.014626539312303066,
-0.008708622306585312,
0.020812438800930977,
0.009786782786250114,
-0.015890780836343765,
0.022114815190434456,
0.008605359122157097,
-0.027571626007556915,
-0.026128387078642845,
0.05638176575303078,
0.05386924743652344,
0.00044010396231897175,
0.005020543001592159,
... |
by the english poet william blake some two centuries ago contains the following four lines : to see the world in a grain of sand and a heaven in a wild flower hold infinity in the palm of your hand and eternity in an hour integrated concepts the problem set for this section involves concepts from this chapter and sever... | openstax_college_physics_2e-web_7zesafu | [
-0.019841928035020828,
0.010207678191363811,
0.018420802429318428,
-0.013972672633826733,
-0.020358502864837646,
0.013482792302966118,
0.007942898198962212,
-0.02737264148890972,
0.02902226708829403,
0.032138802111148834,
0.024996278807520866,
0.02756900154054165,
0.03229953348636627,
-0.0... |
29. 8 β’ the particle - wave duality reviewed 1307 β’ electric potential and electric field β’ electric current, resistance, and ohm β s law β’ wave optics β’ special relativity example 29. 10 illustrates how these strategies are applied to an integrated - concept problem. example 29. 10 recoil of a dust particle after abso... | openstax_college_physics_2e-web_7zesafu | [
0.0072952513583004475,
-0.012050098739564419,
0.008166717365384102,
0.00711634149774909,
-0.050973813980817795,
-0.011858691461384296,
-0.04657377302646637,
-0.020845621824264526,
-0.022264210507273674,
0.09346716105937958,
0.010926060378551483,
0.04410091042518616,
0.03856794536113739,
-0... |
29. 53 1308 29 β’ quantum physics access for free at openstax. org solution for ( b ) conservation of momentum in the absorption of this photon by a grain of dust can be analyzed using the equation : the net external force is zero, since the dust is in outer space. let 1 represent the photon and 2 the dust particle. bef... | openstax_college_physics_2e-web_7zesafu | [
0.013103235512971878,
-0.004896408412605524,
0.028045350685715675,
0.015324859879910946,
-0.003966162912547588,
-0.01712750643491745,
-0.039888013154268265,
-0.008161963894963264,
-0.0024096197448670864,
0.0452643558382988,
0.01064244657754898,
0.03359745815396309,
0.02955949865281582,
-0.... |
29. 8 β’ the particle - wave duality reviewed 1309 glossary atomic spectra the electromagnetic emission from atoms and molecules binding energy also called the work function ; the amount of energy necessary to eject an electron from a material blackbody an ideal radiator, which can radiate equally well at all wavelength... | openstax_college_physics_2e-web_7zesafu | [
-0.017301127314567566,
-0.01215661596506834,
0.04052114486694336,
0.013282114639878273,
-0.020734036341309547,
0.004218237474560738,
-0.02359827421605587,
-0.03142828494310379,
-0.08185126632452011,
0.05740036070346832,
0.027210645377635956,
-0.009136036038398743,
0.04131676256656647,
-0.0... |
uv ; ionizing photons slightly more energetic than violet light uncertainty in energy lack of precision or lack of knowledge of precise results in measurements of energy uncertainty in momentum lack of precision or lack of knowledge of precise results in measurements of momentum uncertainty in position lack of precisio... | openstax_college_physics_2e-web_7zesafu | [
0.011172793805599213,
-0.028557900339365005,
0.010969497263431549,
0.008419482968747616,
-0.006544336210936308,
-0.009413023479282856,
-0.019604023545980453,
-0.03032432496547699,
-0.04670926555991173,
0.07159953564405441,
0.013060370460152626,
-0.017832396551966667,
0.030895976349711418,
... |
29. 1 quantization of energy β’ the first indication that energy is sometimes quantized came from blackbody radiation, which is the emission of em radiation by an object with an emissivity of 1. β’ planck recognized that the energy levels of the emitting atoms and molecules were quantized, with only the allowed values of... | openstax_college_physics_2e-web_7zesafu | [
-0.020630111917853355,
-0.021504003554582596,
0.05132365599274635,
0.0076163094490766525,
-0.020708775147795677,
0.002979628276079893,
-0.02801467850804329,
-0.02198144420981407,
-0.0697534903883934,
0.06433844566345215,
-0.015018882229924202,
-0.011773976497352123,
0.03439322113990784,
-0... |
photon. 29. 5 the particle - wave duality β’ em radiation can behave like either a particle or a wave. β’ this is termed particle - wave duality. 29. 6 the wave nature of matter β’ particles of matter also have a wavelength, called the de broglie wavelength, given by, where is momentum. β’ matter is found to have the same ... | openstax_college_physics_2e-web_7zesafu | [
-0.006497325375676155,
-0.0060288612730801105,
0.03431990370154381,
-0.003527298104017973,
-0.019973114132881165,
0.024092109873890877,
-0.019678277894854546,
-0.0205478947609663,
-0.06070353463292122,
0.08628053218126297,
0.03713433817028999,
-0.015361127443611622,
0.026844369247555733,
-... |
of a child β s swing under such circumstances. 5. why don β t we notice quantization in everyday events? | openstax_college_physics_2e-web_7zesafu | [
-0.00864615011960268,
0.02066410705447197,
0.006554190069437027,
0.03803044185042381,
-0.011714395135641098,
-0.0412076860666275,
-0.019116351380944252,
0.009182935580611229,
-0.005357527639716864,
0.04439806193113327,
0.021445395424962044,
-0.01175377145409584,
0.0038183301221579313,
0.00... |
Subsets and Splits
No community queries yet
The top public SQL queries from the community will appear here once available.