10,944 research outputs found

    Random geometric phase sequence due to topological effects in our brane world from extra dimensions

    Full text link
    Using Kaluza-Klein theory we discuss the quantum mechanics of a particle in the background of a domain wall (brane) embedded in extra dimensions. We show that the geometric phases associated with the particle depend on the topological features of those spacetimes. Using a cohomological modeling schema, we deduce a random phase sequence composed of the geometric phases accompanying the periodic evolution over the spacetimes. The random phase sequence is demonstrated some properties that could be experimental verification. We argue that it is related to the nonlocality of quantum entanglement.Comment: 8 pages, no figure

    Pseudorandom Phase Ensemble and Nonlocal

    Full text link
    In this paper, we introduce a new conception of pseudorandom phase ensemble to simulate a quantum ensemble. A pseudorandom sequence is inseparability and integral that are demonstrated only for a whole sequence not for a single phase unit, which is similar to that of quantum ensembles and a quantum particle. By using the ensemble conception, we demonstrate non-locality properties for classical fields similar to quantum entanglement.Comment: New versions. Correct spelling and grammatical errors. 11 pages, no figure

    Spectrum of jet emitting disc: Application to microquasar XTE J1118+480

    Full text link
    Under the framework of the magnetized accretion ejection structures, we analyze the energy balance properties, and study the spectral energy distributions (SEDs) of the Jet Emitting Disc (JED) model for black hole X-ray transients. Various radiative processes are considered, i.e. synchrotron, bremsstrahlung, and their Comptonizations, and external Comptonization of radiation from outer thin disc. With these cooling terms taken into account, we solve the thermal equilibrium equation self-consistently and find three solutions, of which the cold and the hot solutions are stable. Subsequently we investigate the theoretical SEDs for these two stable solutions.We find the hot JED model can naturally explain the spectra of the Galactic microquasars in their hard states. As an example, we apply this model to the case of XTE J1118+480.Comment: 10 pages, 6 figures. Accepted for the publication in MNRA

    Numerical simulation of Bell inequality's violation using optical transverse modes in multimode waveguides

    Full text link
    We numerically demonstrate that "mode-entangled states" based on the transverse modes of classical optical fields in multimode waveguides violate Bell's inequality. Numerically simulating the correlation measurement scheme of Bell's inequality, we obtain the normalized correlation functions of the intensity fluctuations for the two entangled classical fields. By using the correlation functions, the maximum violations of Bell's inequality are obtained. This implies that the two classical fields in the mode-entangled states, although spatially separated, present a nonlocal correlation.Comment: 10 pages, 5 figures, some typos corrected and two fig replace

    Relations between the Kahler cone and the balanced cone of a Kahler manifold

    Full text link
    In this paper, we consider a natural map from the Kahler cone to the balanced cone of a Kahler manifold. We study its injectivity and surjecticity. We also give an analytic characterization theorem on a nef class being Kahler.Comment: Some corrects have been mad

    Instability of three-band Tomonaga-Luttinger liquid: renormalization group analysis and possible application to K2Cr3As3

    Full text link
    Motivated by recently discovered quasi-one-dimensional superconductor K2_{2}Cr3_{3}As3_{3} with D3hD_{3h} lattice symmetry, we study one-dimensional three-orbital Hubbard model with generic electron repulsive interaction described by intra-orbital repulsion UU, inter-orbital repulsion, and Hund's coupling JJ. As extracted from density functional theory calculation, two of the three atomic orbitals are degenerate (E′E^{\prime} states) and the third one is non-degenerate (A1′A^{\prime}_1), and the system is presumed to be at an incommensurate filling. With the help of bosonization, we have usual three-band Tomonaga-Luttinger liquid for the normal state. Possible charge density wave (CDW), spin density wave (SDW) and superconducting (SC) instabilities are analyzed by renormalization group. The ground state depends on the ratio J/UJ/U and is sensitive to the degeneracy of E′E^{\prime} bands. At 0<J<U/30<J<U/3, spin-singlet SC state is favored, while spin-triplet superconductivity will be favored in the region U/3<J<U/2U/3<J<U/2. The SDW state has the lowest energy only in the unphysical parameter region J>U/2J>U/2. When the two-fold degeneracy of E′E^{\prime} bands is lifted, SDW instability has the tendency to dominate over the spin-singlet SC state at 0<J<U/30<J<U/3, while the order parameter of the spin-triplet SC state will be modulated by a phase factor 2ΔkFx2\Delta k_F x at U/3<J<U/2U/3<J<U/2. Possible experimental consequences and applications to K2_{2}Cr3_{3}As3_{3} are discussed.Comment: two more appendices are adde

    Electron transport with re-acceleration and radiation in the jets of X-ray binaries

    Full text link
    This paper studies acceleration processes of background thermal electrons in X-ray binary jets via turbulent stochastic interactions and shock collisions. By considering turbulent magnetized jets mixed with fluctuation magnetic fields and ordered, large-scale one, and numerically solving the transport equation along the jet axis, we explore the influence of such as magnetic turbulence, electron injections, location of an acceleration region, and various cooling rates on acceleration efficiency. The results show that (1) the existence of the dominant turbulent magnetic fields in the jets is necessary to accelerate background thermal electrons to relativistic energies. (2) Acceleration rates of electrons depend on magnetohydrodynamic turbulence types, from which the turbulence type with a hard slope can accelerate electrons more effectively. (3) An effective acceleration region should be located at the distance >103Rg>10^3R_{\rm g} away from the central black hole (RgR_{\rm g} being a gravitational radius). As a result of acceleration rates competing with various cooling rates, background thermal electrons obtain not only an increase in their energies but also their spectra are broadened beyond the given initial distribution to form a thermal-like distribution. (4) The acceleration mechanisms explored in this work can reasonably provide the electron maximum energy required for interpreting high-energy γ\gamma-ray observations from microquasars, but it needs to adopt some extreme parameters in order to predict a possible very high-energy γ\gamma-ray signal.Comment: 13 pages, 9 figures and 2 tables. Accepted for publication in Monthly Notices of the Royal Astronomical Societ

    Effective Simulation of Quantum Entanglement Based on A Single-photon Field Modulated with Pseudorandom Phase Sequences

    Full text link
    We demonstrate that a single-photon field modulated with n different pseudorandom phase sequences (PPSs) can constitute a 2^n-dimensional Hilbert space that contains tensor product structure. By using the single photon field modulated with PPSs, we discuss effective simulation of Bell states and GHZ state, and apply both correlation analysis and von Neumann entropy to characterize the simulation. We obtain similar results with the cases in quantum mechanics and find that the conclusions can be easily generalized to n quantum particles. The research on simulation of quantum entanglement may be important, for it not only provides useful insights into fundamental features of quantum entanglement, but also yields new insights into quantum computation.Comment: 5 pages, 3 figures, a major corrected version. Added an important appendix in which we propose three theoretical prediction

    Perturbative treatment for stationary state of local master equation

    Full text link
    The local approach to construct master equation for a composite open system with a weak internal coupling is simple and seems reasonable. However, it is thermodynamic consistent only when the subsystems are resonantly coupled. Efforts are being made to understand the inconsistency and test the validity of the local master equation. We present a perturbative method to solve the steady-state solutions of linear local master equations, which are demonstrated by two simple models. The solving process shows the stationary state as the result of competition between incoherent operations and the unitary creating quantum coherence, and consequently relate quantum coherence with thermodynamic consistency.Comment: 5 pages, no fi

    Explicit BCJ numerators of nonlinear sigma model

    Full text link
    In this paper, we investigate the color-kinematics duality in nonlinear sigma model (NLSM). We present explicit polynomial expressions for the kinematic numerators (BCJ numerators). The calculation is done separately in two parametrization schemes of the theory using Kawai-Lewellen-Tye relation inspired technique, both lead to polynomial numerators. We summarize the calculation in each case into a set of rules that generates BCJ numerators for all multilplicities. In Cayley parametrization we find the numerator is described by a particularly simple formula solely in terms of momentum kernel.Comment: 32 pages, 2 figures; v2: typos fixed, references added, matches published versio
    • …
    corecore