14,468 research outputs found
Error estimates of numerical methods for the nonlinear Dirac equation in the nonrelativistic limit regime
We present several numerical methods and establish their error estimates for
the discretization of the nonlinear Dirac equation in the nonrelativistic limit
regime, involving a small dimensionless parameter which is
inversely proportional to the speed of light. In this limit regime, the
solution is highly oscillatory in time, i.e. there are propagating waves with
wavelength and in time and space, respectively. We
begin with the conservative Crank-Nicolson finite difference (CNFD) method and
establish rigorously its error estimate which depends explicitly on the mesh
size and time step as well as the small parameter . Based on the error bound, in order to obtain `correct' numerical solutions
in the nonrelativistic limit regime, i.e. , the CNFD method
requests the -scalability: and
. Then we propose and analyze two numerical methods
for the discretization of the nonlinear Dirac equation by using the Fourier
spectral discretization for spatial derivatives combined with the exponential
wave integrator and time-splitting technique for temporal derivatives,
respectively. Rigorous error bounds for the two numerical methods show that
their -scalability is improved to and
when compared with the CNFD method. Extensive
numerical results are reported to confirm our error estimates.Comment: 35 pages. 1 figure. arXiv admin note: substantial text overlap with
arXiv:1504.0288
Prospects for Detecting Neutrino Signals from Annihilating/Decaying Dark Matter to Account for the PAMELA and ATIC results
Recent PAMELA data show that positron fraction has an excess above several
GeV while anti-proton one is not. Moreover ATIC data indicates that
electron/positron flux have a bump from 300 GeV to 800 GeV. Both annihilating
dark matter (DM) with large boost factor and decaying DM with the life around can account for the PAMELA and ATIC observations if their main final
products are charged leptons (, and ). In this work, we
calculated the neutrino flux arising from and which originate from
annihilating/decaying DM, and estimated the final muon rate in the neutrino
telescopes, namely Antares and IceCube. Given the excellent angular resolution,
Antares and IceCube are promising to discover the neutrino signals from
Galactic center and/or large DM subhalo in annihilating DM scenario, but very
challenging in decaying DM scenario.Comment: 21 pages, 7 figures, 2 tables. V2: references added. V3: the number
density of massive subhalo has been discussed in the appendix; accepted by
PR
A fourth-order compact time-splitting method for the Dirac equation with time-dependent potentials
In this paper, we present an approach to deal with the dynamics of the Dirac
equation with time-dependent electromagnetic potentials using the fourth-order
compact time-splitting method (). To this purpose, the
time-ordering technique for time-dependent Hamiltonians is introduced, so that
the influence of the time-dependence could be limited to certain steps which
are easy to treat. Actually, in the case of the Dirac equation, it turns out
that only those steps involving potentials need to be amended, and the scheme
remains efficient, accurate, as well as easy to implement. Numerical examples
in 1D and 2D are given to validate the scheme.Comment: 24pages, 8 figure
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