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MASS CHARGE GROUPING & |
in MeV —e 0 +e STRANGENESS |
1400p= Y[>AJtT- YỊ3A}LT? VỈ›AẰI s=-2 |
T395 |
=_- =0 S=-2 |
1300 1319 TBIT |
1200 _— >° >+ s=-llố |
1196 1191 "T189 È |
Ạ9 S=_-1|m |
1100 1115 |
—n - mi S=0 |
839 938 |
s00 023m S=0 |
Đ—OT‡T 271m7 p°©X‡T S=0 |
500 _KC KT gr s=ml| 2 |
494 498 494 õ |
TT— r0 ii S=0 |
T39.6 Tâ5Ø 139.6 |
_H—— œ |
100 T0B.6 z |
0 B5 ~8— |
--- Trang 66 --- |
mass, within one or two percent. Each particle in a multiplet has the same |
strangeness. The first multiplet is the proton-neutron doublet, and then there is |
a singlet (the lambda) then the sigma triplet, and ñnally the xi doublet. Very |
recenfly, in 1961, even a few more particles were found. Ôr are they particles? |
They live so short a time, they disintegrate almost instantaneouslÌy, as soon as |
they are formed, that we do not know whether they should be considered as new |
particles, or some kind of “resonance” interaction of a certain definite energy |
between the Á and z produects into which they disintegrate. |
In addition to the baryons the other particles which are involved in the nuclear |
interaction are called rmesons. “Thore are first the pions, which come in three |
varleties, positive, negative, and neutral; they form another multiplet. We have |
also found some new things called K-mesons, and they occur as a doublet, KT |
and K0. Also, every particle has its antiparticle, unless a particle is is ơun |
antiparticle. Eor example, the x— and the z? are antiparticles, but the #2 is |
its own antiparticle. The K~ and KT are antiparticles, and the KU and KD. |
In addition, in 1961 we also found some more mesons or ?nø;/be mmesons which |
disintegrate almost immediately. A thing called œ¡ which goes into three pions |
has a mass 780 on this scale, and somewhat less certain is an object which |
disintegrates into two pions. These particles, called mesons and baryons, and |
the antiparticles of the mesons are on the same chart, but the antiparticles of |
the baryons must be put on another chart, “reflected” through the charge-zero |
column. |
Just as Mendeleev's chart was very good, except for the fact that there were |
a number oŸ rare earth elements which were hanging out loose from it, so we have |
a number of things hanging out loose from this chart—particles which do not |
interact strongly in nuclei, have nothing to do with a nuclear interaction, and do |
not have a strong interaction (I mean the powerful kind of interaction of nuclear |
energy). These are called leptons, and they are the following: there is the electron, |
which has a very small mass on this scale, only 0.510 MeV. Then there is that |
other, the /-meson, the muon, which has a mass mụch higher, 206 times as heavy |
as an electron. So far as we can tell, by all experiments so far, the diference |
bebween the electron and the muon is nothing but the mass. Everything works |
exactly the same for the muon as for the electron, except that one is heavier than |
the other. Why is there another one heavier; what is the use for it? We do not |
know. In addition, there is a lepton which is neutral, called a neutrino, and this |
particle has zero mass. In fact, it is now known that there are £#o diferent kinds |
of neutrinos, one related to electrons and the other related to muons. |
--- Trang 67 --- |
Pinally, we have two other particles which do not interact strongly with the |
nuclear ones: one is a photon, and perhaps, If the field of gravity also has a |
quantum-mechanical analog (a quantum theory of gravitation has not yet been |
worked out), then there will be a particle, a graviton, which will have zero mass. |
What is this “zero mass”? "he masses given here are the masses of the |
particles ø‡ resf. The fact that a particle has zero mass means, in a way, that it |
cannot be at resf. Á photon is never at rest, i is always moving at 186,000 miles |
a second. We will understand more what mass means when we understand the |
theory of relativity, which will come in due time. |
Thus we are confronted with a large number of particles, which together seem |
to be the fundamental constituents of matter. Fortunately, these particles are |
not all diferent in their zn#eraclions with one another. In fact, there seem to be |
Just ƒour kinds of interaction between particles which, in the order of decreasing |
strength, are the nuclear force, electrical interactions, the beta-decay interaction, |
and gravity. The photon is coupled to all charged particles and the strength of the |
interaction is measured by some number, which is 1/137. The detailed law of this |
coupling is known, that is quantum electrodynamics. Gravity is coupled to all |
cnergu, but its coupling is extremely weak, much weaker than that of electricity. |
This law is also known. Then there are the so-called weak decays——beta. decay, |
which causes the neutron to disintegrate into proton, electron, and neutrino, |
relatively slowly. This law is only partly known. The so-called strong interaction, |
the meson-baryon interaction, has a strength of 1 in this scale, and the law 1s |
completely unknown, although there are a number of known rules, such as that |
the number of baryons does not change in any reaction. |
Table 2-3. Elementary Interactions |
Coupling Strength” Law |
Photon to charged particles ~ 1072 Law known |
Gravity to all energy ~ 10? Law known |
'Weak decays ~10" Law partly known |
Mesons to baryons ~1 Law unknown (some rules known) |
” The “strength” is a dimensionless measure of the coupling constant involved |
in each interaction (~ means “of the order”). |
--- Trang 68 --- |
This then, is the horrible condition of our physics today. To summarize it, |
I would say this: outside the nucleus, we seem to know all; inside it, quantum |
mmechanics is valid——the principles of quantum mechanies have not been found to |
fail. The stage on which we put all of our knowledge, we would say, is relativistic |
space-time; perhaps gravity is involved in space-time. We do not know how the |
universe got started, and we have never made experiments which check our ideas |
OŸ space and time accurately, below some tỉny distance, so we only knou that our |
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