id stringlengths 9 10 | abstract stringlengths 13 3.93k | embedding list |
|---|---|---|
1001.0001 | The Krotov combining construction of perfect 1-error-correcting binary codes from 2000 and a theorem of Heden saying that every non-full-rank perfect 1-error-correcting binary code can be constructed by this combining construction is generalized to the $q$-ary case. Simply, every non-full-rank perfect code $C$ is the u... | [
-0.015585657209157002,
0.016744695603847,
-0.014822055585682002,
-0.021612657234072002,
-0.025117043405771002,
0.007990547455847001,
-0.0015007843030610001,
-0.033080320805311,
-0.025062501430511003,
-0.027816921472549,
-0.0014505024300880002,
0.039052776992321,
-0.016867417842149002,
0.00... |
1001.0002 | Logarithmic conformal field theories with vanishing central charge describe systems with quenched disorder, percolation or dilute self-avoiding polymers. In these theories the energy momentum tensor acquires a logarithmic partner. In this talk we address the construction of possible gravity duals for these logarithmic ... | [
0.004695892333984,
0.01996518112719,
0.0027995395939790003,
-0.007442802656441001,
0.0007342636818060001,
0.030124336481094003,
-0.020399797707796003,
-0.030395971611142002,
-0.010919732041656001,
-0.014288007281720002,
0.027733946219086,
0.029798373579978003,
-0.009059031493961001,
0.0201... |
1001.0003 | We construct new families of non-supersymmetric sourceless type IIA AdS4 vacua on those coset manifolds that also admit supersymmetric solutions. We investigate the spectrum of left-invariant modes and find that most, but not all, of the vacua are stable under these fluctuations. Generically, there are also no massless... | [
-0.0005790717550550001,
0.004832370672374,
-0.009515740908682001,
-0.008235687389969,
-0.027199441567063002,
0.023162869736552003,
-0.028228901326656,
-0.012360303662717,
0.0037588868290180004,
-0.017351834103465,
0.021754134446382002,
0.013775812461972,
-0.010924476198852002,
0.0290687251... |
1001.0004 | Examples of symmetric informationally complete positive operator valued measures (SIC-POVMs) have been constructed in every dimension less than or equal to 67. However, it remains an open question whether they exist in all finite dimensions. A SIC-POVM is usually thought of as a highly symmetric structure in quantum st... | [
0.023628670722246004,
0.00021616531012100002,
0.022768700495362,
-0.037319920957088006,
-0.033497836440801,
0.030003359541296,
-0.024311184883117003,
-0.024201981723308,
-0.015056281350553001,
-0.029457347467541,
0.026891091838479,
0.017390482127666,
-0.011534503661096,
0.02154017426073500... |
1001.0005 | We aim to reveal environmental dependence of infrared luminosity functions (IR LFs) of galaxies at z~0.8 using the AKARI satellite. We construct restframe 8um IR LFs in the cluster region RXJ1716.4+6708 at z=0.81, and compare them with a blank field using the AKARI North Ecliptic Pole deep field data at the same redshi... | [
0.021031482145190003,
0.007450645789504001,
-0.011589893139898002,
-0.006280709523707,
-0.011152022518217002,
0.027407977730035,
-0.035467535257339006,
-0.002709325635805,
-0.01588650047779,
-0.027572179213166,
0.0015334030613300001,
0.007861149497330001,
0.01052258349955,
0.00342086586169... |
1001.0006 | We present the first comparison of virial masses of galaxy clusters with their Sunyaev-Zel'dovich Effect (SZE) signals. We study 15 clusters from the Hectospec Cluster Survey (HeCS) with MMT/Hectospec spectroscopy and published SZE signals. We measure virial masses of these clusters from an average of 90 member redshif... | [
-0.009176731109619,
-0.007445912342518001,
0.0035939933732150003,
-0.025887612253427002,
-0.017552534118294,
0.040154986083507004,
-0.023118302226066003,
0.010194859467446001,
-0.028263244777917,
-0.049304563552141,
-0.0037263499107210002,
0.042326990514993,
0.0016985775437200002,
0.018027... |
1001.0007 | We reveal cosmic star-formation history obscured by dust using deep infrared observation with the AKARI. A continuous filter coverage in the mid-IR wavelength (2.4, 3.2, 4.1, 7, 9, 11, 15, 18, and 24um) by the AKARI satellite allows us to estimate restframe 8um and 12um luminosities without using a large extrapolation ... | [
0.019308622926473,
-0.0065242024138560005,
-0.018979499116539,
-0.018019553273916,
-0.002357009565457,
0.008872641250491,
-0.028716091066598,
-0.0036717923358080004,
-0.019966870546340002,
-0.018787508830428002,
0.015386559069156001,
0.012273591943085001,
0.007796130608767,
-0.003208961337... |
1001.0008 | In this Letter, we briefly review the multi-stream inflation scenario, and discuss its implications in the string theory landscape and the inflationary multiverse. In multi-stream inflation, the inflation trajectory encounters bifurcations. If these bifurcations are in the observable stage of inflation, then interestin... | [
-0.020563460886478,
-0.0077112978324290005,
-0.003916688263416001,
-0.013286219909787001,
-0.002027861075475,
0.007351844105869001,
-0.034236263483762006,
0.018501689657568002,
-0.031631920486688,
-0.0017870949814090002,
0.012404541485011002,
0.007256893906742,
-0.008355601690709001,
0.028... |
1001.0009 | Theoretical studies of stretching proteins with slipknots reveal a surprising growth of their unfolding times when the stretching force crosses an intermediate threshold. This behavior arises as a consequence of the existence of alternative unfolding routes that are dominant at different force ranges. Responsible for l... | [
-0.018460078164935,
-0.012798245996236001,
0.010370752774178002,
-0.026737205684185004,
-0.013959825970232001,
0.020032037049531,
-0.018627012148499003,
0.0013728552730750002,
-0.037866115570068005,
-0.010516819544136,
0.00862490478903,
0.0019075645832340002,
0.014982294291257001,
0.021687... |
1001.0011 | Spatial separation of electrons and holes in graphene gives rise to existence of plasmon waves confined to the boundary region. Theory of such guided plasmon modes within hydrodynamics of electron-hole liquid is developed. For plasmon wavelengths smaller than the size of charged domains plasmon dispersion is found to b... | [
-0.008414856158196002,
0.022923229262232003,
0.011329719796776001,
-0.001989955315366,
-0.0028159432113170004,
0.011870486661791002,
-0.024967590346932002,
-0.017594698816537,
-0.035769734531641,
-0.013440028764307001,
-0.0033088983036570004,
0.00039320986252200005,
-0.018188223242759,
0.0... |
1001.0012 | [Abridged] If both the day-side and night-side effective temperatures of a planet can be measured, it is possible to estimate its Bond albedo, 0<A_B<1, as well as its day-night heat redistribution efficiency, 0<epsilon<1. We attempt a statistical analysis of the albedo and redistribution efficiency for 24 transiting ex... | [
0.014126621186733001,
0.00617782305926,
-0.010021801106631001,
-0.036407969892024,
-0.004290154669433,
0.028170872479677003,
-0.024217065423727,
0.0011660640593610001,
-0.029900662600994003,
-0.023324713110923,
-0.005048654042184001,
0.015883868560194,
-0.007447708863765,
0.017325360327959... |
1001.0013 | Dust-obscured star-formation becomes much more important with increasing intensity, and increasing redshift. We aim to reveal cosmic star-formation history obscured by dust using deep infrared observation with the AKARI. We construct restframe 8um, 12um, and total infrared (TIR) luminosity functions (LFs) at 0.15<z<2... | [
0.010245432145893001,
-0.004603960085660001,
-0.018593309447169002,
-0.016368119046092002,
0.001377092557959,
0.010347818024456001,
-0.031780634075403005,
-0.004952072631567,
-0.024736473336815,
-0.022784311324357,
0.014074671082198,
0.008914412930607001,
0.009235222823917,
0.0035937507636... |
1001.0014 | Jet shapes are weighted sums over the four-momenta of the constituents of a jet and reveal details of its internal structure, potentially allowing discrimination of its partonic origin. In this work we make predictions for quark and gluon jet shape distributions in N-jet final states in e+e- collisions, defined with a ... | [
-0.017578911036252,
-0.00402620434761,
-0.0035853539593510004,
-0.027291396632790003,
-0.000715520931407,
-0.005879153963178001,
-0.021904755383729,
-0.0015093961264930002,
-0.035020057111978004,
-0.017964655533432003,
0.022070074453949002,
0.008596583269536,
-0.026271929964423003,
0.01324... |
1001.0015 | We conduct a comprehensive analysis of the relationship between central galaxies and their host dark matter halos, as characterized by the stellar mass-halo mass (SM-HM) relation, with rigorous consideration of uncertainties. Our analysis focuses on results from the abundance matching technique, which assumes that ever... | [
-0.0025821144226930003,
0.00250843539834,
0.000308740185573,
-0.032499141991138,
-0.019745975732803,
0.014508066698908001,
-0.027194252237677,
0.0031112637370820004,
-0.0203488022089,
-0.030061036348342004,
0.010750437155365,
0.006992808077484001,
-0.006523941643536001,
0.01604862883687000... |
1001.0016 | Using localization, matrix model and saddle-point techniques, we determine exact behavior of circular Wilson loop in N=2 superconformal (quiver) gauge theories. Focusing at planar and large `t Hooft couling limits, we compare its asymptotic behavior with well-known exponential growth of Wilson loop in N=4 super Yang-Mi... | [
-0.010191120207309001,
0.002086275722831,
0.005475825630128,
-0.0007125660195010001,
-0.016330681741237002,
-0.012859893962740001,
-0.012272210791707,
-0.0046530691906800006,
-0.006626993883401,
-0.023853028193116,
-0.004780976567417001,
-0.0006671934388570001,
-0.017658155411481,
0.032937... |
1001.0017 | We give a test that can distinguish efficiently between product states of n quantum systems and states which are far from product. If applied to a state psi whose maximum overlap with a product state is 1-epsilon, the test passes with probability 1-Theta(epsilon), regardless of n or the local dimensions of the individu... | [
0.014474469237029,
0.009861957281827,
-0.010344905778765,
-0.030096817761659,
-0.011898742057383001,
0.008476103655993,
-0.019961889833211,
-0.010225918143987002,
-0.036760114133358,
-0.025561297312378002,
0.010575881227850002,
0.014320485293865001,
0.0007401717011810001,
0.008042149245738... |
1001.0018 | We study the power of nonadaptive quantum query algorithms, which are algorithms whose queries to the input do not depend on the result of previous queries. First, we show that any bounded-error nonadaptive quantum query algorithm that computes some total boolean function depending on n variables must make Omega(n) que... | [
0.000378588534658,
0.0035135748330500003,
0.00975196249783,
-0.015365486964583001,
-0.017427876591682,
0.025390613824129,
-0.030812924727797,
-0.009021248668432002,
-0.043460428714752,
-0.006760814227163001,
0.024816969409585003,
0.013050420209765,
0.012811401858925,
0.001040584989823,
-... |
1001.0019 | Recent numerical investigations have uncovered a surprising result: Reissner-Nordstrom-de Sitter black holes are unstable for spacetime dimensions larger than 6. Here we prove the existence of such instability analytically, and we compute the timescale in the near-extremal limit. We find very good agreement with the pr... | [
-0.000318771431921,
-0.008071484044194001,
0.019830800592899,
-0.029447000473737002,
-0.008704678155481,
-0.004547168035060001,
-0.029252171516418003,
-0.010819963179528,
-0.013978974893689001,
-0.004453232511878001,
0.016003804281353,
0.007549620699137001,
0.0049368259496980005,
0.0172701... |
1001.0021 | To analyze the ground-state phase diagram of Bose-Bose mixtures loaded into $d$-dimensional hypercubic optical lattices, we perform a strong-coupling power-series expansion in the kinetic energy term (plus a scaling analysis) for the two-species Bose-Hubbard model with onsite boson-boson interactions. We consider both ... | [
-0.014143070206046,
0.000871253781951,
0.00458127213642,
-0.024862028658390004,
0.004906089045107,
0.017837863415479,
-0.0019793531391760003,
-0.019759695976972,
-0.024090589955449,
-0.04336306080222101,
0.007829441688954001,
0.026594387367367002,
-0.0016790666850280001,
0.0010032106656580... |
1001.0022 | Motivated by large nu_mu-nu_tau flavor mixing, we consider mu-tau production at hadron colliders via dimension-6 effective operators, which can be attributed to new physics in the flavor sector at a higher scale Lambda. Current bounds on many of these operators from low energy experiments are very weak or nonexistent, ... | [
-0.011542682535946001,
-0.016122229397296,
-0.020722625777125,
-0.028825435787439003,
-0.011931840330362,
-0.002281086985021,
-0.04694904759526201,
-0.008478069677948001,
-0.05959665775299001,
-0.02305756881833,
0.014996454119682001,
0.028964420780539003,
-0.019596848636865002,
-0.01346067... |
1001.0023 | If $X$ is a smooth manifold then the $\mathbb R$-algebra $C^\infty(X)$ of smooth functions $c:X\to\mathbb R$ is a $C^\infty$-$ring$. That is, for each smooth function $f:{\mathbb R}^n\to\mathbb R$ there is an $n$-fold operation $\Phi_f:C^\infty(X)^n\to C^\infty(X)$ acting by $\Phi_f:(c_1,\ldots,c_n)\mapsto f(c_1,...,c_... | [
0.011757467873394,
0.012728142552077002,
-0.002271173754706,
-0.033604484051465,
-0.018278760835528002,
0.014136304147541,
-0.012598264031112002,
-0.004227903671562,
-0.005796705372631001,
-0.033713854849338004,
0.026303917169570003,
0.0029137330129740003,
0.005885569844394,
0.013322851620... |
1001.0024 | The hybrid Monte Carlo (HMC) algorithm is applied for the Bayesian inference of the stochastic volatility (SV) model. We use the HMC algorithm for the Markov chain Monte Carlo updates of volatility variables of the SV model. First we compute parameters of the SV model by using the artificial financial data and compare ... | [
-0.011047637090086,
-0.008642990142107001,
-0.010353724472224001,
-0.02219146117568,
-0.004902045708149,
0.013019448146224001,
-0.013555341400206,
-0.00041608986794000006,
-0.03382995352149,
-0.030037481337785003,
-0.006399797275662001,
0.039463698863983,
0.017890576273202,
0.0105048744007... |
1001.0025 | Increasing numbers of mobile computing devices, user-portable, or embedded in vehicles, cargo containers, or the physical space, need to be aware of their location in order to provide a wide range of commercial services. Most often, mobile devices obtain their own location with the help of Global Navigation Satellite S... | [
-0.021956726908683003,
0.018349647521972,
0.0022988296113900003,
0.006322635803371001,
-0.011169647797942,
0.00252427207306,
-0.04129012301564201,
-0.007193663157522001,
-0.01963398605585,
-0.004218506161123001,
0.031698573380708,
0.01986626163125,
-0.015466718003153001,
0.012064586393535,... |
1001.0026 | Asteroseismology of stars in clusters has been a long-sought goal because the assumption of a common age, distance and initial chemical composition allows strong tests of the theory of stellar evolution. We report results from the first 34 days of science data from the Kepler Mission for the open cluster NGC 6819 -- on... | [
0.009014149196445,
-0.008069227449595,
-0.006441106088459001,
-0.032168142497539,
-0.00039725820533900003,
0.030971692875027,
-0.012596696615219002,
0.008096419274806001,
-0.015757767483592002,
-0.01001345552504,
-0.010917589999735001,
0.019836567342281,
0.00864705722779,
0.008667451329529... |
1001.0027 | We present the results of the search for candidate Planetary Nebulae interacting with the interstellar medium (PN-ISM) in the framework of the INT Photometric H$\alpha$ Survey (IPHAS) and located in the right ascension range 18h-20h. The detection capability of this new Northern survey, in terms of depth and imaging re... | [
-0.004007388371974,
-0.0034598375204950003,
0.0018274512840430002,
-0.015304049476981002,
-0.030142679810523,
0.036959689110517,
-0.018958952277898,
0.002896886784583,
-0.022586476057767,
-0.002660755300894,
0.016768747940659003,
0.004202453419566,
0.011799722909927,
0.013688773848116,
-... |
1001.0028 | We present the proof of the cyclic sieving conjectures for generalised non-crossing partitions associated to well-generated complex reflection groups due to Armstrong, respectively to Bessis and Reiner, for the 26 exceptional well-generated complex reflection groups. The computational details are provided in the manusc... | [
-0.010629982687532001,
0.020059693604707003,
-0.0032041706144800004,
0.000237984684645,
0.008381200022995,
0.037774033844470006,
-0.019066367298364,
0.00042962271254500005,
-0.014596394263207002,
-0.013954870402812002,
0.024336520582437002,
0.013823806308209001,
-0.007891434244811,
0.00850... |
1001.0029 | In 1979 Louis Witten demonstrated that stationary axially symmetric Einstein field equations and those for static axially symmetric self-dual SU(2) gauge fields can both be reduced to the same (Ernst) equation. In this paper we use this result as point of departure to prove the existence of the mass gap for quantum sou... | [
-0.005776507314294001,
0.015476679429411002,
-0.006427045445889,
0.004690005909651,
-0.010994437150657,
-0.002840570174157,
-0.02713868394494,
-0.011382716707885002,
-0.009393636137247,
-0.038882430642843004,
0.008187926374375001,
0.014495762996375,
0.0015420480631290001,
0.030817121267318... |
1001.0031 | Exact analytic expressions for planetary orbits and light trajectories in the Schwarzschild geometry are presented. A new parameter space is used to characterize all possible planetary orbits. Different regions in this parameter space can be associated with different characteristics of the orbits. The boundaries for th... | [
0.015033024363219,
0.0069165392778810005,
0.0027521220035850004,
-0.025926910340785002,
-0.008581631816923,
0.027639193460345,
-0.014507205225527,
-0.028798690065741,
-0.025401093065738,
-0.008750163950026,
0.012511790730059001,
0.009134416468441,
-0.007840093225240001,
0.005386271979659,
... |
1001.0032 | In addition to its great potential for characterizing extra-solar planetary systems the Kepler mission is providing unique data on stellar oscillations. A key aspect of Kepler asteroseismology is the application to solar-like oscillations of main-sequence stars. As an example we here consider an initial analysis of dat... | [
0.017952797934412002,
0.0008883598493410001,
-0.0076535614207380006,
-0.015482601709663,
-0.014537717215716001,
0.035419657826423,
-0.015685077756643,
0.003062437055632,
-0.010913412086665,
-0.0035163189750160003,
0.015442106872797002,
0.020530981943011003,
-0.001110238838009,
0.0228661969... |
1001.0033 | We present 5201 radial-velocity measurements of 1144 stars, as part of an ongoing study of the young (150 Myr) open cluster M35 (NGC 2168). We have observed M35 since 1997, using the Hydra Multi-Object Spectrograph on the WIYN 3.5m telescope. Our stellar sample covers main-sequence stars over a magnitude range of 13.0<... | [
-0.019704977050423,
0.010541284456849001,
0.002696097129955,
-0.028524270281195002,
-0.017476517707109,
0.038923744112253,
-0.022649243474006,
0.0065739527344700005,
-0.030550140887498002,
-0.035196140408515,
-0.015680244192481003,
0.033467397093772,
-0.009832229465246001,
0.00858294218778... |
1001.0034 | In this paper we give new identities involving q-Euler polynomials of higher order. | [
0.0018771389732130002,
0.031249636784195,
-0.015935424715280002,
-0.012593036517500001,
-0.011438393965363001,
0.006428188178688001,
-0.015408745035529001,
-0.004125654231756,
-0.0019176527857780001,
0.007447785232216001,
0.026941670104861003,
0.0011082210112360001,
-0.001449212082661,
0.0... |
1001.0035 | In [1], the spectrum (eigenvalues and eigenstates) of a lattice regularizations of the Sine-Gordon model has been completely characterized in terms of polynomial solutions with certain properties of the Baxter equation. This characterization for cyclic representations has been derived by the use of the Separation of Va... | [
0.011283011175692002,
-0.000638701487332,
0.0070827663876110005,
-0.013307639397680001,
-0.026244668290019,
0.024858312681317003,
-0.011358506046235001,
0.000455541303381,
-0.031350851058959,
0.0032788678072390005,
0.034398086369037004,
0.025846606120467002,
-0.007762217894196,
0.032998003... |
1001.0036 | Neurons perform computations, and convey the results of those computations through the statistical structure of their output spike trains. Here we present a practical method, grounded in the information-theoretic analysis of prediction, for inferring a minimal representation of that structure and for characterizing its... | [
-0.010068903677165,
0.021342517808079,
0.017440902069211003,
-0.015182072296738002,
-0.0029159437399350003,
0.005400656256824001,
0.005383543670177,
-0.019891390576958,
-0.021575244143605003,
-0.042794551700353005,
0.007111890707165,
0.038934007287025,
-0.009788261726498,
0.022862093523144... |
1001.0037 | The notion of textile system was introduced by M. Nasu in order to analyze endomorphisms and automorphisms of topological Markov shifts. A textile system is given by two finite directed graphs $G$ and $H$ and two morphisms $p,q:G\to H$, with some extra properties. It turns out that a textile system determines a first q... | [
-0.011629287153482002,
-0.010451813228428001,
-0.004398211836814,
0.008083012886345001,
0.0077990335412320005,
0.007771328557282001,
-0.020072469487786,
-0.010597266256809,
0.00850551854819,
-0.036460135132074,
0.004522885661572,
0.004851885605603,
0.0035566641017790003,
0.0265416502952570... |
1001.0038 | In this paper we study ``Bergman-type'' singular integral operators on Ahlfors regular metric spaces. The main result of the paper demonstrates that if a singular integral operator on a Ahlfors regular metric space satisfies an additional estimate, then knowing the ``T(1)'' conditions for the operator imply that the op... | [
0.010517691262066,
-0.005017456132918,
0.008234835229814,
-0.029187455773353,
-0.00177421385888,
0.024138962849974,
-0.023035468533635,
0.0040174131281670005,
-0.027035638689994004,
-0.024401044473052,
0.017117973417043002,
0.018414581194519,
0.006717528682202,
0.016166208311915002,
-0.0... |
1001.0039 | The recently released Chandra Transmission Grating Catalog and Archive, TGCat, presents a fully dynamic on-line catalog allowing users to browse and categorize Chandra gratings observations quickly and easily, generate custom plots of resulting response corrected spectra on-line without the need for special software an... | [
-0.007946773432195001,
0.0014367097755890001,
0.005064468830823001,
-0.045832552015781,
0.009844616055488,
0.011543435044586001,
-0.014770478941500001,
-0.025588894262909,
-0.021125053986907002,
-0.012232912704348,
0.009254650212824001,
0.007189768366515001,
-0.0047055133618410004,
0.00474... |
1001.0041 | It has been known since 1970's that the N-dimensional $\ell_1$-space contains nearly Euclidean subspaces whose dimension is $\Omega(N)$. However, proofs of existence of such subspaces were probabilistic, hence non-constructive, which made the results not-quite-suitable for subsequently discovered applications to high-d... | [
0.021129878237843,
0.0061123752966520005,
0.003075127489864,
-0.027397215366363,
0.0022538308985530003,
0.006852747406810001,
-0.013374910689890001,
0.002856459468603,
-0.031928982585668,
-0.026102425530552004,
0.010675134137272,
0.004466338548809,
-0.009504313580691,
-0.001747622853145,
... |
1001.0042 | We construct new seven-dimensional gravity by adding two topological terms to the Einstein-Hilbert action. For certain choice of the coupling constants, these terms may be related to the R^4 correction to the 3-form field equation of eleven-dimensional supergravity. We derive the full set of the equations of motion. We... | [
0.00031548028346100004,
0.003186771413311,
0.006824469193816,
-0.016125669702887,
-0.008668556809425,
0.004307357128709,
-0.035131882876157004,
-0.011851962655782,
-0.007807085290551001,
-0.027647849172353002,
0.019167739897966,
0.010310736484825,
0.005364005919545001,
0.015250736847519002... |
1001.0043 | We present new radial velocity measurements of the ultra-cool dwarf VB 10, which was recently announced to host a giant planet detected with astrometry. The new observations were obtained using optical spectrographs(MIKE/Magellan and ESPaDOnS/CHFT) and cover a 63% of the reported period of 270 days. We apply Least-squa... | [
-0.024096295237541,
0.0036213288549330003,
-0.011042987927794,
-0.021948281675577,
-0.031366489827632,
0.028364781290292,
-0.028612628579139,
-0.00003988259413745254,
-0.030953411012887004,
-0.011600644327700001,
-0.005741802975535001,
0.036874216049909,
-0.015104934573173,
0.0176522564142... |
1001.0044 | When modelling metapopulation dynamics, the influence of a single patch on the metapopulation depends on the number of individuals in the patch. Since the population size has no natural upper limit, this leads to systems in which there are countably infinitely many possible types of individual. Analogous considerations... | [
0.008048203773796,
0.019094228744506,
0.018972694873809003,
-0.017811378464102003,
-0.017541304230690002,
0.010850220918655,
-0.011883254162967,
0.004807316698133,
-0.024374173954129,
-0.030599379912018002,
0.017757363617420002,
0.002818896900862,
0.0034907059744,
0.015839837491512,
0.00... |
1001.0045 | In this work the analysis of mixing parameters of the system involving eta, eta' mesons and some third massive state G is carried out. We use the generalized mixing scheme with three angles. The framework of the dispersive approach to Abelian axial anomaly of isoscalar non-singlet current and the analysis of experiment... | [
-0.017270987853407003,
0.010825554840266,
-0.007471157237887001,
-0.027819318696856003,
-0.024451060220599,
0.0037113216239950003,
-0.027902485802769002,
-0.014956176280975002,
-0.016799708828330002,
-0.014651230536401001,
0.007526602130383001,
0.017659099772572,
-0.022884750738739003,
0.0... |
1001.0046 | The Cayley graph construction provides a natural grid structure on a finite vector space over a field of prime or prime square cardinality, where the characteristic is congruent to 3 modulo 4, in addition to the quadratic residue tournament structure on the prime subfield. Distance from the null vector in the grid grap... | [
0.006165786646306,
-0.002419614465907,
-0.0011556620011100001,
-0.019113261252641,
-0.013387405313551001,
0.006605716422200001,
-0.009861198253929001,
-0.014402627944946001,
-0.019438132643699,
-0.043045450001955005,
0.015593823045492,
0.010889956727623001,
-0.017570123076438002,
0.0083451... |
1001.0047 | We obtain and analyze the effect of electron-electron Coulomb interaction on the time dependent current flowing through a mesoscopic system connected to biased semi-infinite leads. We assume the contact is gradually switched on in time and we calculate the time dependent reduced density operator of the sample using the... | [
-0.028490522876381003,
0.004733609966933,
0.01825088635087,
-0.032619185745716005,
-0.012659416534006,
0.009884187951683,
-0.007874540053308001,
-0.017430622130632,
-0.05725446715950901,
-0.019918758422136,
0.008824679069221,
0.034888584166765005,
-0.0038723321631550004,
0.016514658927917,... |
1001.0048 | Extending results of Oh and Zumbrun in dimensions $d\ge 3$, we establish nonlinear stability and asymptotic behavior of spatially-periodic traveling-wave solutions of viscous systems of conservation laws in critical dimensions $d=1,2$, under a natural set of spectral stability assumptions introduced by Schneider in the... | [
0.004098279401659,
0.019677285104990002,
0.00006966511864447966,
-0.00042048070463300005,
-0.005234573502093,
0.015520111657679001,
-0.012014228850603001,
-0.023585027083754,
-0.0047287838533520005,
-0.022947592660784003,
0.012388374656438002,
0.014563961885869002,
0.027520483359694002,
0.... |
1001.0049 | The Swift Burst Alert Telescope (BAT) survey of Active Galactic Nuclei (AGN) is providing an unprecedented view of local AGNs (<z> = 0.03) and their host galaxy properties. In this paper, we present an analysis of the optical spectra of a sample of 64 AGNs from the 9-month survey, detected solely based on their 14-195 ... | [
0.001472159288823,
-0.005157345905900001,
-0.014918345026671002,
-0.010621136985719001,
-0.010753466747701002,
0.029028788208961,
-0.018484260886907,
0.006445811595767001,
-0.026493644341826002,
-0.024376381188631002,
0.027677638456225003,
0.015976976603269,
0.0010307726915920001,
-0.00734... |
1001.0051 | We discuss the thermal evolution and Bose-Einstein condensation of ultra-light dark matter particles at finite, realistic cosmological temperatures. We find that if these particles decouple from regular matter before Standard model particles annihilate, their temperature will be about 0.9 K. This temperature is substan... | [
0.007580397184938001,
-0.001082188100554,
-0.0036242292262610005,
-0.025064762681722003,
-0.015255633741617002,
0.007099424954503001,
-0.028153825551271,
-0.008400082588195001,
-0.017396301031112,
-0.024698952212929,
-0.0043389135971660005,
0.038261022418737,
-0.014754339121282002,
0.00788... |
1001.0052 | The phase-integral method (PIM) is an asymptotic method of the geometrical optics or semi-classical type for solving approximately, but in many cases very accurately, a wide class of differential equations in physics. Unlike the related (J)WKB method, the higher-order corrections in the PIM can be generated from a gene... | [
0.008976086042821001,
0.01046869251877,
-0.0087716197595,
-0.008137772791087001,
-0.018061222508549,
0.031760487705469,
-0.00694164307788,
-0.034513972699642,
-0.018088484182953002,
-0.018347475677728,
0.038657829165458006,
0.019206235185265,
0.00043832539813500005,
0.017515977844595,
-0... |
1001.0053 | Rotation vectors, as defined for homeomorphisms of the torus that are isotopic to the identity, are generalized to such homeomorphisms of any complete Riemannian manifold with non-positive sectional curvature. These generalized rotation vectors are shown to exist for almost every orbit of such a dynamical system with r... | [
-0.014649042859673,
-0.015482290647923001,
-0.014958150684833001,
-0.017215983942151,
0.0025652623735360003,
0.00040297466330200003,
-0.013459648005664002,
0.0041024037636810005,
-0.002212475752457,
-0.029513116925954003,
0.025024328380823004,
0.007479075342416001,
-0.014635602943599,
0.00... |
1001.0054 | There is currently an intersection in the research of game theory and cryptography. Generally speaking, there are two aspects to this partnership. First there is the application of game theory to cryptography. Yet, the purpose of this paper is to focus on the second aspect, the converse of the first, the application of... | [
-0.013519381172955001,
-0.0046195699833330005,
0.006262456998229001,
-0.025533623993396003,
0.010798035189509001,
0.007787755224853,
-0.007673525717109,
0.0019486186793070002,
-0.0036419010721140004,
-0.031527306884527005,
0.028086986392736,
0.00394763238728,
-0.003253857139497,
0.01403005... |
1001.0055 | Fortuin-Kastelyn clusters in the critical $Q$-state Potts model are conformally invariant fractals. We obtain simulation results for the fractal dimension of the complete and external (accessible) hulls for Q=1, 2, 3, and 4, on clusters that wrap around a cylindrical system. We find excellent agreement between these re... | [
0.011436742730438001,
-0.0037345178425310004,
-0.0042809476144610005,
-0.026019807904958003,
-0.0036997133865950002,
0.020409330725669,
-0.022497598081827,
-0.006271762307733001,
-0.017318695783615,
-0.026423539966344,
0.015216506086289001,
0.019587945193052,
0.014395121484994002,
0.017485... |
1001.0056 | Let G denote a complex, semisimple, simply-connected group. We identify the equivariant quantum differential equation for the cotangent bundle to the flag variety of G with the affine Knizhnik-Zamolodchikov connection of Cherednik and Matsuo. This recovers Kim's description of quantum cohomology of the flag variety its... | [
-0.003126874100416,
0.011324169114232,
0.00015296830679200002,
-0.003011637367308,
-0.007237561047077,
0.027753157541155003,
-0.022483222186565,
0.014819113537669001,
0.0064223036170000004,
-0.027725638821721,
0.014530161395668002,
0.026377195492386003,
0.01350506953895,
0.019442345947027,... |
1001.0057 | We present a generic mechanism by which reproducing microorganisms, with a diffusivity that depends on the local population density, can form stable patterns. It is known that a decrease of swimming speed with density can promote separation into bulk phases of two coexisting densities; this is opposed by the logistic l... | [
-0.010399687103927,
0.026775261387228,
0.005828884430229,
-0.013996159657835001,
-0.010023629292845001,
0.027404302731156002,
0.003938342910259,
0.022262576967477,
-0.022905291989445003,
-0.041079103946685,
0.009182629175484,
0.019746413454413,
0.017872964963316,
0.025900075212121003,
0.... |
1001.0058 | The $C$-function of $T$-adic exponential sums is studeid. An explicit arithmetic bound is established for the Newton polygon of the $C$-function. This polygon lies above the Hodge polygon. It gives a sup-Hodge bound of the $C$-function of $p$-power order exponential sums. | [
0.009406547993421001,
0.01661523990333,
0.012924499809741,
0.0035801555495700004,
-0.028558306396007004,
0.0013883470091960001,
-0.009213025681674,
-0.024646399542689,
-0.00568125071004,
-0.016131434589624002,
0.024867566302418,
0.017181981354951,
0.013843728229403001,
0.016573769971728002... |
1001.0059 | The TANAMI (Tracking AGN with Austral Milliarcsecond Interferometry) and associated programs provide comprehensive radio monitoring of extragalactic gamma-ray sources south of declination -30 degrees. Joint quasi-simultaneous observations between the Fermi Gamma-ray Space Telescope and ground based observatories allow ... | [
-0.009356218390166001,
-0.018519951030611003,
-0.006912327371537,
-0.013927772641181,
-0.012305386364459001,
0.029367940500378,
-0.037699855864048004,
-0.007039505988359,
-0.021833468228578002,
-0.014615224674344,
0.012697233818471002,
0.012697233818471002,
-0.002304682042449,
-0.008338790... |
1001.0061 | The energy density of the Universe is dominated by dark energy and dark matter, two mysterious components which pose some of the most important questions in fundamental science today. Euclid is a high-precision survey mission designed to answer these questions by mapping the geometry of the dark Universe. Euclid's Visi... | [
0.033846803009510006,
0.007791331503540001,
-0.0031021675094960004,
-0.031958822160959,
0.0017580089624970002,
0.025104640051722003,
-0.021410770714282,
-0.025241451337933003,
-0.009364646859467,
-0.028538573533296002,
0.009624585509300001,
-0.004617338534444001,
-0.006741314195096,
0.0156... |
1001.0062 | Unfolded equations of motion for symmetric massive bosonic fields of any spin in Minkowski and (A)dS spaces are presented. Manifestly gauge invariant action for a spin $s \ge 2$ massive field in any dimension is constructed in terms of gauge invariant curvatures. | [
-0.021759700030088,
-0.014457337558269001,
-0.011054034344851001,
0.004622596316039,
-0.01312415394932,
-0.0005564701277760001,
-0.026717266067862,
-0.005781595129519,
-0.007818217389285,
-0.026958445087075,
0.013961580581963002,
0.002421838464215,
0.010913346894085001,
0.026275105774402,
... |
1001.0063 | In this paper we give a thorough presentation of a model proposed by Tononi et al. for modeling \emph{integrated information}, i.e. how much information is generated in a system transitioning from one state to the next one by the causal interaction of its parts and \emph{above and beyond} the information given by the s... | [
-0.012458964250981001,
0.020835950970649,
0.010926504619419,
-0.01698762178421,
-0.015626963227987,
-0.000119508644274,
-0.012726972810924001,
0.004463374149054,
-0.023103715851902,
-0.040050104260444,
0.01295374892652,
0.029219809919595004,
-0.0041163372807200005,
0.016190467402338,
0.0... |
1001.0064 | In this paper, we develop some of the theory of SSD spaces and SSDB spaces, and deduce some results on maximally monotone multifunctions on a reflexive Banach space. | [
-0.004639245104044,
0.013154657557606001,
0.008900327607989,
-0.018867613747715003,
-0.01935382373631,
0.019016178324818,
-0.020758427679538,
0.006256565451622001,
-0.015234551392495,
-0.011932381428778002,
0.015842312946915002,
0.014316156506538,
0.019907562062144002,
0.011304361745715,
... |
1001.0065 | Magnetic field in the solar lower atmosphere can be measured by the use of the Zeeman and Hanle effects. In contrast, the coronal magnetic field well above the solar surface, which directly controls various eruptive phenomena, can not be precisely measureed with the traditional techniques. Several attempts are being ma... | [
-0.016557751223444002,
0.007731784135103,
0.008746869862079001,
-0.036463964730501,
-0.025851711630821003,
0.015463568270206,
-0.031217161566019003,
-0.015068081207573001,
-0.003951581194996,
-0.009821278043091,
-0.009742179885506,
0.024981638416647002,
-0.013202697038650001,
0.01711143366... |
1001.0066 | We investigate a matter dominated navigation cosmological model. The influence of a possible drift (wind) in the navigation cosmological model makes the spacetime geometry change from Riemannian to Finslerian. The evolution of the Finslerian Universe is governed by the same gravitational field equation with the familia... | [
0.025887044146656,
0.00718624331057,
0.013564811088144,
-0.0035206379834560003,
-0.010334108024835,
0.005063505843281,
-0.030291292816400004,
0.006489018909633001,
-0.0050980220548800005,
-0.040231917053461005,
0.002000205684453,
0.013792617246508002,
0.019121896475553003,
0.02632884867489... |
1001.0067 | We demonstrate an efficient numerical method to calculate three-tangle of general mixed states. We construct a "energy function" (target function) for the three-tangle of the mixed state under certain constrains. The "energy function" (target function) is then optimized via a replica exchange Monte Carlo method. We hav... | [
-0.017416687682271,
-0.010821550153195001,
0.011463798582553001,
-0.007727705407887001,
-0.00419533625245,
0.008079906925559,
-0.014460960403084,
-0.0037360934074960003,
-0.037706229835748006,
-0.024792192503809003,
-0.00336144817993,
0.02686396241188,
0.0015857679536560002,
0.013369828462... |
1001.0068 | Bayesian methods since the time of Laplace have been understood by their practitioners as closely aligned to the scientific method. Indeed a recent champion of Bayesian methods, E. T. Jaynes, titled his textbook on the subject Probability Theory: the Logic of Science. Many philosophers of science including Karl Popper ... | [
-0.013773337006568001,
0.0031096711754790003,
0.001094143604859,
-0.011104032397270001,
-0.009972627274692001,
0.012987449765205002,
-0.015690628439188,
-0.001654765103012,
-0.005718001164495,
-0.027289226651191004,
-0.010412994772195,
0.026706587523221,
-0.003827808657661,
0.0230887997895... |
1001.0069 | Physical-layer Network Coding (PNC) makes use of the additive nature of the electromagnetic (EM) waves to apply network coding arithmetic at the physical layer. With PNC,the destructive effect of interference in wireless networks is eliminated and the capacity of networks can be boosted significantly. This paper addres... | [
0.005432225298136,
0.002541372086852,
0.019557368010282003,
-0.008387546055018002,
0.003667854703962,
0.005632413551211001,
-0.024212591350078003,
-0.001148537266999,
-0.041856296360492005,
-0.021240305155515,
0.011366616934537001,
0.026112683117389002,
-0.005941178184002,
0.00566295068711... |
1001.0071 | An all-sky comprehensive catalog of calculated radio and X-ray associations to optical objects is presented. Included are X-ray sources from XMM-Newton, Chandra and ROSAT catalogs, radio sources from NVSS, FIRST and SUMSS catalogs, and optical data, identifications and redshifts from the APM, USNO-A, SDSS-DR7 and the e... | [
0.007623176090419001,
0.014528877101838,
0.007857735268771001,
-0.048677947372198,
-0.047215402126312006,
0.028202302753925,
-0.007154057733714,
0.003340744879096,
-0.023331748321652003,
-0.013776907697319,
0.0018919964786610001,
-0.011341630481183002,
-0.013563044369220002,
0.009216799400... |
1001.0072 | Polya Enumeration Theorem is one of the most useful tools dealing with the enumeration of patterns that are symmetric in some ways. What follows is a procedure for obtaining the results of Polya Theorem directly, bypassing the usual preliminaries. | [
-0.014700132422149001,
0.004034942016005,
-0.008109507150948,
-0.029928572475910003,
-0.029928572475910003,
0.017117135226726,
-0.023602100089192002,
-0.0065774177201090005,
-0.012956720776855,
-0.014620887115597002,
0.021000189706683003,
-0.010552925989031,
0.010434056632220001,
0.0032309... |
1001.0073 | We show that for a $\sigma $-ideal $\ci$ with a Steinhaus property defined on Banach space, if two non-homeomorphic Banach with the same cardinality of the Hamel basis then there is a $\ci$ nonmeasurable subset as image by any isomorphism between of them. Our results generalize results from [2] | [
-0.008092877455055,
-0.014043921604752001,
-0.0028111564461140003,
-0.018015801906585003,
-0.0075235292315480005,
0.018503814935684003,
-0.019886517897248,
0.013250900432467001,
-0.007896317169070001,
-0.021540338173508002,
-0.0019317170372230002,
0.011122623458504,
0.005280026234686001,
0... |
1001.0074 | We explain how Lie superalgebras of types gl and osp provide a natural framework generalizing the classical Schur and Howe dualities. This exposition includes a discussion of super duality, which connects the parabolic categories O between classical Lie superalgebras and Lie algebras. Super duality provides a conceptua... | [
0.020313909277319003,
0.048628620803356004,
0.0066311759874220005,
-0.044506173580884004,
-0.019066326320171002,
0.016842372715473,
0.003410512814298,
-0.007051557302474001,
0.001728987554088,
-0.033874593675136004,
0.004251275211572,
0.031623519957065,
-0.010109491646289001,
0.03308807685... |
1001.0075 | We prove that the class of principal coactions is closed under one-surjective pullbacks in an appropriate category of algebras equipped with left and right coactions. This allows us to handle cases of C*-algebras lacking two different non-trivial ideals. It also allows us to go beyond the category of comodule algebras.... | [
0.012812552042305001,
0.014163821004331001,
0.013764741830527002,
-0.020752133801579,
-0.025233026593923003,
0.020612105727195,
-0.004785453435033,
-0.004134323447942,
0.0054750903509550005,
-0.035147000104188,
-0.006570809055119001,
0.023552691563963002,
0.014030794613063,
0.0186517145484... |
1001.0076 | GLACIER (Giant Liquid Argon Charge Imaging ExpeRiment) is a large underground observatory for proton decay search, neutrino astrophysics and CP-violation studies in the lepton sector. Possible underground sites are studied within the FP7 LAGUNA project (Europe) and along the JPARC neutrino beam in collaboration with KE... | [
0.0007356107234950001,
-0.012214559130370001,
0.006552067585289,
-0.030683521181344004,
0.001907455734908,
0.009142101742327,
-0.031860496848821,
0.007725622970610001,
-0.010873353108763001,
-0.025387123227119,
0.00434865662828,
0.016806138679385,
-0.016149220988154002,
-0.0083620119839900... |
1001.0077 | The feasibility of a next generation neutrino observatory in Europe is being considered within the LAGUNA design study. To accommodate giant neutrino detectors and shield them from cosmic rays, a new very large underground infrastructure is required. Seven potential candidate sites in different parts of Europe and at s... | [
0.009787550196051,
-0.011110937222838001,
0.017176462337374,
-0.006289535202085,
0.002157396636903,
0.013571610674262002,
-0.026150681078433,
-0.010966191999614001,
-0.013978276401758001,
-0.009704838506877,
0.005958688445389,
-0.0029466040432450003,
0.005793265067040001,
-0.00511433975771... |
1001.0078 | We extend the matrix decomposition method(MDM) in classifying the $2\times N\times N$ truly entangled states to $2\times M\times N$ system under the condition of stochastic local operations and classical communication. It is found that the MDM is quite practical and convenient in operation for the asymmetrical triparti... | [
-0.014485986903309002,
0.025722526013851003,
-0.014363109134137,
-0.035334341228008,
0.000354981777491,
0.024794112890958002,
-0.032112199813127004,
-0.006055170204490001,
-0.036399286240339,
-0.013530267402529002,
0.008785799145698001,
0.042952794581651,
-0.006567162927240001,
0.016001487... |
1001.0079 | Based on perturbation theory, we study the dynamics of how dark matter and dark energy in the collapsing system approach dynamical equilibrium while interacting. We find that the interaction between dark sectors cannot ensure the dark energy to fully cluster along with dark, leading to the energy non-conservation probl... | [
-0.005878811702132,
-0.00864828005433,
0.0021889908239240002,
-0.02121352404356,
0.011104796081781,
0.022371115162968,
-0.031174190342426,
-0.00537741323933,
-0.02048666588962,
-0.011273049749433,
0.018777200952172002,
0.014483345672488001,
-0.001057479414157,
0.025776585564017,
-0.00432... |
1001.0081 | In the present work we explore electron transport properties through a quantum interferometer attached symmetrically to two one-dimensional semi-infinite metallic electrodes, namely, source and drain. The interferometer is made up of two sub-rings where individual sub-rings are penetrated by Aharonov-Bohm fluxes $\phi_... | [
-0.016740493476390002,
0.001336264424026,
0.003097058041021,
-0.007708381861448001,
-0.006702214013785001,
0.023706784471869,
-0.013197177089750002,
-0.013043411076068,
-0.024923544377088002,
-0.026795485988259003,
0.007541244383901,
0.004843644797801,
0.002177801681682,
0.0192274991422890... |
1001.0082 | Detailed comparisons are reported between laboratory observations of electron-scale dissipation layers near a reconnecting X-line and direct two-dimensional full-particle simulations. Many experimental features of the electron layers, such as insensitivity to the ion mass, are reproduced by the simulations; the layer t... | [
-0.015156625770032002,
0.029109476134181002,
0.005745291244238,
-0.013227849267423,
-0.015854267403483002,
0.0014559867559000002,
0.006733618211001001,
-0.006716519128531001,
-0.042186852544546,
-0.02458163909614,
0.007653548847883,
0.027604756876826002,
0.001202065381221,
0.01017737295478... |
1001.0083 | We present a study of tau->pipipinu, tau->Kpipinu, tau->KKpinu, and tau->KKKnu decays using a 666 fb-1 data sample collected with the Belle detector at the KEKB asymmetric-energy e+e- collider at and near a center-of-mass energy of 10.58 GeV. The branching fractions are measured to be: B(tau->pipipinu) = (8.42+-0.01+0.... | [
-0.014259782619774002,
-0.011510169133543,
0.008630921132862,
-0.037034496665,
-0.020618690177798,
0.0007428391836580001,
-0.028164776042103,
0.0015351440524680002,
-0.019881822168827,
-0.032422244548797004,
0.007921343669295,
0.021996909752488,
-0.008126029744744,
-0.0023590046912430004,
... |
1001.0084 | We consider a time independent Schrodinger type equation derived from the equations of motion that drives a single scalar field in a standard cosmology model for inflation in a flat space-time with a Friedman-Robertson-Walker (FRW) metric with a cosmological constant. We find that all the 1-dimensional bound state solu... | [
0.022915510460734003,
0.007834934629499,
-0.007667521480470001,
-0.013794842176139,
-0.014598425477743001,
-0.013634125702083002,
-0.021013697609305,
-0.016861850395798,
-0.015428794547915,
-0.023478018119931002,
0.011176501400768,
0.027750400826334003,
0.014102882705628001,
0.033830847591... |
1001.0085 | In this short paper, we show a certain matrix trace inequality and then give a refinement of the trace inequality proven by Belmega, Lasaulce and Debbah. In addition, we give an another improvement of their trace inequality. | [
-0.011088334023952,
0.007977021858096001,
-0.00006569349352503195,
-0.035499114543199005,
-0.000755983812268,
0.004074174445122001,
-0.028317056596279002,
0.007154648192226,
-0.020216677337884,
-0.007188913878053001,
0.015707330778241,
0.007915343157947001,
0.001404031179845,
-0.0042831944... |
1001.0086 | We show that the maximum slope invariant for tubular groups is easy to calculate, and give an example of two tubular groups that are distinguishable by their maximum slopes but not by edge pattern considerations or isoperimetric function. | [
-0.00024361856048900002,
0.016576880589127003,
0.014433203265070001,
-0.013301448896527,
0.003525083651766,
0.010458746924996001,
-0.0009012430673460001,
-0.0034851392265400002,
-0.013993816450238,
-0.00047267408808600005,
0.010618523694574,
0.0062579386867580005,
0.025843955576419,
0.0289... |
1001.0087 | We discuss the information that can be obtained from an analysis of fluctuations in heavy ion collisions within the context of the statistical model of particle production. We then examine the recently published experimental data on ratio fluctuations, and use it to obtain constraints on the statistical properties (phy... | [
-0.021285332739353003,
0.007279692217707001,
0.0035453045275060002,
-0.046433359384536,
0.002517166314646,
0.0046899314038450005,
-0.013749028556048001,
0.014194724150002001,
-0.028173353523015,
-0.032684329897165,
0.015680376440286,
0.024810379371047003,
-0.011723140254616,
0.008002258837... |
1001.0088 | A careful look at an allegedly well-known century-old concept reveals interesting aspects in it that have generally avoided recognition in literature. There are four different kinds of physical observables known or proclaimed as relativistic invariants under space-time rotations. Only observables in the first three cat... | [
0.023609599098563003,
-0.008564266376197,
-0.004663372412323,
-0.016556674614548,
-0.0012756196083500001,
-0.0031435214914380004,
-0.014160313643515,
-0.024412924423813,
-0.029300956055521004,
-0.008911466225981001,
0.021594477817416,
0.015018101781606001,
-0.011382712982594,
0.00552796851... |
1001.0089 | We describe a method to enhance the sensitivity of precision measurements that takes advantage of a quantum sensor's environment to amplify its response to weak external perturbations. An individual qubit is used to sense the dynamics of surrounding ancillary qubits, which are in turn affected by the external field to ... | [
-0.023450378328561002,
0.015163195319473001,
0.015356885269284002,
-0.014429938048124001,
-0.00828718394041,
0.040702663362026006,
-0.022412750869989003,
-0.026839962229132003,
-0.038267698138952005,
-0.024709366261959003,
0.012264755554497,
0.030271049588918002,
-0.010964263230562,
0.0176... |
1001.0091 | Making use of the Lagrange anchor construction introduced earlier to quantize non-Lagrangian field theories, we extend the Noether theorem beyond the class of variational dynamics. | [
-0.003905261633917,
0.003250456880778,
0.00987088587135,
-0.001824699807912,
0.014409068971872002,
0.010867400094866001,
-0.057205349206924,
-0.013870411552488,
-0.009237963706254002,
-0.020913349464535002,
-0.002742099575698,
0.023889428004622,
0.018543260172009003,
0.016105838119983,
0... |
1001.0092 | A general feature of TeV-scale radiative seesaw models, in which tiny neutrino masses are generated via loop corrections, is an extended scalar (Higgs) sector. Another feature is the Majorana nature; e.g., introducing right-handed neutrinos with TeV-scale Majorana masses under the discrete symmetry, or otherwise introd... | [
-0.013785109855234002,
-0.001003819634206,
0.0057579502463340005,
-0.007738413289189,
-0.014892539009451,
0.00122802297119,
-0.024526489898562,
-0.008764313533902,
-0.025898886844515003,
-0.038834739476442004,
0.012059424072504,
0.013581288978457002,
-0.016061114147305003,
0.00786750018596... |
1001.0093 | By analysing the Chandra and XMM-Newton archived data of the nearby galaxy cluster Abell 3158, which was reported to possess a relatively regular, relaxed morphology in the X-ray band in previous works, we identify a bow edge-shaped discontinuity in the X-ray surface brightness distribution at about $120h_{71}^{-1}$ kp... | [
-0.0007209144532680001,
0.00833745766431,
0.016564667224884002,
-0.027024388313293003,
-0.028967497870326,
0.021429333835840003,
-0.015944527462124002,
-0.007800001651048,
-0.012099649757146001,
-0.022876329720020003,
0.010824914090335001,
-0.000159018920385,
0.01285070925951,
0.0166335720... |
1001.0094 | In this article we prove the existence of a stochastic optimal transference plan for a stochastic Monge-Kantorovich problem by measurable selection theorem. A stochastic version of Kantorovich duality and the characterization of stochastic optimal transference plan are also established. Moreover, Wasserstein distance b... | [
0.0019119575154030002,
-0.01954598352313,
0.017909128218889,
-0.020866472274065,
0.015639537945389,
0.02273716405034,
-0.013026070781052002,
0.006141647696495001,
-0.036891151219606004,
-0.019848594442009003,
0.006282637361437001,
0.039669681340456,
-0.006145086605101001,
0.014869252219796... |
1001.0095 | Asymptotics of the variances of many cost measures in random digital search trees are often notoriously messy and involved to obtain. A new approach is proposed to facilitate such an analysis for several shape parameters on random symmetric digital search trees. Our approach starts from a more careful normalization at ... | [
-0.0022893103305250003,
0.008577581495046002,
0.005561971571296001,
-0.010468375869095001,
-0.011186049319803,
0.024042071774601003,
-0.001136029255576,
-0.013214858248829,
-0.039444454014301,
-0.024663135409355,
0.005172081757336001,
0.011910623870790001,
-0.005610276479274001,
0.00881910... |
1001.0096 | Mirror dark matter offers a framework to explain the existing dark matter direct detection experiments, including the impressive DAMA annual modulation signal. Here we examine the implications of mirror dark matter for experiments like CDMSII/Ge and XENON10 which feature higher recoil energy threshold than the DAMA NaI... | [
-0.014463969506323001,
-0.010100536979734,
-0.021345801651477002,
-0.013925273902714001,
-0.018207902088761,
0.020834041759371,
-0.037708673626184006,
-0.008295907638967,
-0.021642085164785,
-0.016632217913866,
0.013884872198104001,
0.026247929781675002,
-0.020416552200913003,
0.0069020339... |
1001.0097 | When the Moon was formed it was much closer to the Earth than it is today. It just needed about 20 days then to go around the Earth. Now it takes the Moon 29.5 days to make one revolution. In order to follow the conservation of angular momentum the Moon had to either move closer to the Earth or recede from Earth. The d... | [
0.0048299715854220006,
0.010497731156647,
0.022188674658536002,
-0.0034685670398170005,
-0.021262031048536002,
-0.027926249429583,
-0.030134961009025,
0.0011717918096110001,
-0.006378609221428,
-0.020259223878383,
0.009025256149470001,
0.022937605157494,
0.006223110482096001,
0.01463589351... |
1001.0098 | We study the dynamics of the relative phase of a bilayer of two-dimensional superfluids after the two superfluids have been decoupled. We find that on short time scales the relative phase shows "light cone" like dynamics and creates a metastable superfluid state, which can be supercritical. We also demonstrate similar ... | [
-0.009136757813394,
0.0034314133226870003,
0.009150435216724,
0.011147391982376001,
0.007256062701344001,
0.01659114845097,
-0.015537959523499002,
-0.000874095712788,
-0.031103273853659002,
-0.036437608301639,
0.020420927554368,
0.011974897235631,
-0.000840328691992,
0.012617752887308,
0... |
1001.0099 | Simultaneous imaging of the piezoresponse phase, amplitude and bare surface topography of displacive ferroelectric thin films by scanning probe microscopy directly shows the nature of domain wall pinning and its relation to morphological disorder. Strong and stable pinning of walls occurs at grain boundaries while weak... | [
-0.007293413858860001,
0.012155690230429,
0.021355878561735,
-0.01062345970422,
-0.020320773124694002,
0.027784433215856,
-0.018645534291863,
-0.007940355688333001,
-0.016806859523057,
-0.045953273773193005,
0.024556536227464003,
0.013429143466055001,
0.027280500158667002,
0.02286767959594... |
1001.0101 | Using the exact solutions for the Dirac neutrino wave function in presence of matter we study the spin light mode in the process of neutrino transition from initial heavier to final lighter state. The spin light is emitted due to the neutrino nonzero transitional magnetic moment. | [
0.020329479128122,
-0.00026726108626400004,
0.0032180503476410003,
0.0064058685675260005,
-0.005952385254204001,
0.008135822601616001,
-0.009560095146298,
-0.016123842447996,
-0.027759883552789,
-0.026483412832021002,
0.012126473709940001,
0.014390530064702001,
-0.010144584812223,
0.007531... |
1001.0102 | In order to study an intrinsic chemical potential jump between the hole- and electron-doped high-Tc superconductors, we have performed core-level X-ray photoemission spectroscopy (XPS) measurements of Y0.38La0.62Ba1.74La0.26Cu3Oy (YLBLCO), into which one can dope both holes and electrons with maintaining the same cryst... | [
-0.005511609371751,
0.001860252581536,
0.024421084672212,
-0.028333855792880003,
-0.019658299162983003,
0.022653592750430003,
-0.016973327845335,
-0.030060870572924003,
-0.034864135086536005,
-0.011326796375215002,
0.014571697451174,
0.017040790989995003,
0.0006324521382330001,
0.008574364... |
1001.0103 | The latest determination of the extragalactic gamma-ray background (EGRB) radiation by Fermi is compared with the theoretical prediction of the blazar component by Inoue & Totani (2009; hereafter IT09). The Fermi EGRB spectrum is in excellent agreement with IT09, indicating that blazars are the dominant component of th... | [
-0.0015506914351130002,
-0.024661762639880003,
-0.022612269967794002,
-0.029534393921494,
-0.004550278186798,
0.016667388379573,
-0.039659697562456006,
-0.025068946182727002,
-0.030945964157581003,
-0.007146074436604001,
0.000799522211309,
0.015011507086455001,
-0.007112142629921001,
0.019... |
1001.0104 | For the first time the process-independent parameter of double parton scattering, $\sigma_{\rm eff}^{\rm exp}$, has been measured newly in the D0 experiment at the three different resolution scales.If we interpret the measurement as a decrease of the effective cross section with a growth of the resolution scale it can ... | [
-0.019882660359144003,
0.007366694509983,
-0.008687711320817,
-0.03890261799097,
-0.020421851426362003,
0.006635416764765,
-0.016270082443952002,
0.0023572747595600003,
-0.043836213648319,
-0.024411862716078002,
0.029574615880846002,
0.012846221216022,
0.001957936678081,
0.0008075224468480... |
1001.0105 | The strong interaction between electrons reveals the duality of the itinerancy and the localization of quasiparticles. The physical phenomena corresponding to each component of the duality could be realized and coexist within the category of the uncertainty principle of the carrier dynamics, which can be a strong reaso... | [
0.009998625144362,
0.009698666632175001,
0.012271646410226001,
-0.020343869924545,
-0.015971137210726002,
0.009358713403344,
-0.027782846242189,
-0.01723762974143,
-0.037354864180088,
-0.0296225938946,
0.012378297746181,
0.015104589983820001,
-0.0012248315615570001,
0.025196535512804003,
... |
1001.0106 | The structural profiles and electronic properties of pentacene (C$_{22}$H$_{14}$) multilayers on Ag(111) surface has been studied within the density functional theory (DFT) framework. We have performed first-principle total energy calculations based on the projector augmented wave (PAW) method to investigate the initia... | [
-0.004579776898026001,
0.000159367235028,
0.000489142839796,
-0.030025202780961,
0.006209697108715001,
0.028078630566596003,
-0.009339544922113,
-0.020612329244613002,
-0.017039168626070002,
-0.015532576479017,
0.003986472263932,
0.03077183291316,
-0.009179552085697,
0.009039559401571001,
... |
1001.0107 | The high repair cost of (n,k) Maximum Distance Separable (MDS) erasure codes has recently motivated a new class of codes, called Regenerating Codes, that optimally trade off storage cost for repair bandwidth. On one end of this spectrum of Regenerating Codes are Minimum Storage Regenerating (MSR) codes that can match t... | [
-0.017726402729749003,
0.016081972047686,
-0.0038706827908750003,
-0.00021763880795300003,
-0.011037194170057002,
0.011134745553135001,
-0.007985242642462,
-0.009671480394899,
-0.017378006130456,
-0.016723021864891,
0.0034491231199350004,
0.043619215488433005,
-0.012214773334562001,
0.0145... |
1001.0108 | Surface waves on a thin metal filament are described in terms of quantum electrodynamics. The interaction of surface waves with a quantum oscillator is discussed in the dipole approximation. The increase in the spontaneous emission rate of the excited quantum oscillator, the so called Purcell factor, is evaluated to be... | [
-0.006425260566174,
0.008219822309911001,
0.003094872459769,
-0.007257857359945,
-0.025780653581023,
0.014701473526656001,
-0.027757655829191003,
-0.011775773949921001,
-0.040734227746725006,
-0.015670072287321,
-0.0102034593001,
0.019265830516815,
-0.006547993980348001,
0.0329588986933230... |
1001.0109 | The formation mechanism of planetesimals in protoplanetary discs is hotly debated. Currently, the favoured model involves the accumulation of meter-sized objects within a turbulent disc, followed by a phase of gravitational instability. At best one can simulate a few million particles numerically as opposed to the seve... | [
-0.010922388173639,
0.009758526459336002,
-0.003532903501763,
-0.020054221153259003,
-0.0072310888208440005,
0.025536075234413,
-0.010571163147687001,
0.011046349070966001,
-0.025012681260704002,
-0.043634455651044006,
0.009193813428282,
0.017519894987344003,
-0.0076925014145670005,
0.0098... |
1001.0111 | This articles presents a simulation study of the applicability of the Rosenfeld entropy scaling to the systems which can not be approximated by effective hard spheres. Three systems are studied: Herzian spheres, Gauss Core Model and soft repulsive shoulder potential. These systems demonstrate the diffusion anomalies at... | [
-0.004947294946759001,
0.006973526440560001,
0.010525430552661,
-0.03881038352847,
0.02339594066143,
0.029046073555946003,
-0.013947052881121,
-0.014495609328150002,
-0.040702901780605004,
-0.040346339344978006,
0.016278417780995,
0.034723635762929,
-0.0024376485962420004,
0.02387592755258... |
Subsets and Splits
No community queries yet
The top public SQL queries from the community will appear here once available.