15,021 research outputs found
Finite linear groups, lattices, and products of elliptic curves
Let be a finite dimensional complex linear space and let be an
irreducible finite subgroup of \GL(V). For a -invariant lattice
in of maximal rank, we give a description of structure of the complex torus
. In particular, we prove that for a wide class of groups,
is isogenous to a self-product of an elliptic curve, and that in
many cases is isomorphic to a product of mutually isogenous
elliptic curves with complex multiplication. We show that there are and
such that the complex torus is not an abelian variety but
one can always replace by another -invariant lattice such
that is a product if elliptic curves with complex multiplication. We
amplify these results with a criterion, in terms of the character and the Schur
-index of -module , of the existence of a nonzero
-invariant lattice in .Comment: 25 pages. Several examples are adde
The experimental study of the surface current excitation under the influence of a relativistic electron electromagnetic field
The problem of the surface current excitation in a conductive targets by a
relativistic electron electric field as the origin of such radiation mechanisms
as diffraction and transition radiation of relativistic electron was considered
in frame of both surface current and pseudo-photon methods. The contradiction
between these viewpoints in respect to the surface current on the target
downstream surface necessitated the experimental test of this phenomenon. The
test performed on electron beam of the 6 MeV microtron showed, that not any
surface current is induced on the target downstream surface under the influence
of a relativistic electron electromagnetic field in contrast to the upstream
surface. This is important implication for the understanding of the forward
transition and diffraction radiation nature.Comment: Was Presented at the symposium Channeling 2008 (Charged and Neutral
Particles Channeling Phenomena), October 25 - November 1, 2008 Erice (Trapani
- Sicily), Italy, and was accepted for publication in proceedings of
symposiu
Parametric study of the conditions of supershear crack propagation in brittle materials
This article may be downloaded for personal use only. Any other use requires prior permission of the author and AIP Publishing. This article appeared in AIP Conference Proceedings 1683, 020209 (2015) and may be found at https://doi.org/10.1063/1.4932899.The paper is devoted to the numerical analysis of the conditions of acceleration of dynamically propagating longitudinal shear cracks from sub-Rayleigh to intersonic/supershear velocities. We showed that an ability of the initial crack to propagate in supershear regime can be predicted with use of the empirically derived dependence of the geometrical criterion of sub-Raleigh-to-intersonic transition on material and crack parameters
Schwinger Pair Creation of Particles and Strings
I shortly review the worldline instanton method for calculating Schwinger
pair production rates in (i) one-loop QED (ii) multiloop QED and (iii) one-loop
open string theory.Comment: 8 pages, 3 figures, talk given at XIV Mexican School of Particles and
Fields, November 8 - 12, 2010, Morelia, Mexico, to appear in the conference
proceeding
Thermodynamic Properties of Kagome Lattice in ZnCu_3(OH)_6Cl_2 Herbertsmithite
Strongly correlated Fermi systems are among the most intriguing and
fundamental systems in physics, whose realization in some compounds is still to
be discovered. We show that herbertsmithite ZnCu_3(OH)_6Cl_2 can be viewed as a
strongly correlated Fermi system whose low temperature thermodynamic in
magnetic fields is defined by a quantum critical spin liquid. Our calculations
of its thermodynamic properties are in good agreement with recent experimental
facts and allow us to reveal their scaling behavior which strongly resembles
that observed in HF metals and 2D 3He.Comment: 4 pages, 6 figure
A young contracting white dwarf in the peculiar binary HD 49798/RX J0648.0--4418?
HD 49798/RX J0648.0--4418 is a peculiar X-ray binary with a hot subdwarf
(sdO) mass donor. The nature of the accreting compact object is not known, but
its spin period ~s and s~s, prove
that it can be only either a white dwarf or a neutron star. The spin-up has
been very stable for more than 20 years. We demonstrate that the continuous
stable spin-up of the compact companion of HD 49798 can be best explained by
contraction of a young white dwarf with an age ~Myrs. This allows us to
interpret all the basic parameters of the system in the framework of an
accreting white dwarf. We present examples of binary evolution which result in
such systems. If correct, this is the first direct evidence for a white dwarf
contraction on early evolutionary stages.Comment: 9 pages, accepted to MNRA
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