4,665 research outputs found
Noncommutative Residues and a Characterisation of the Noncommutative Integral
We continue the study of the relationship between Dixmier traces and
noncommutative residues initiated by A. Connes. The utility of the residue
approach to Dixmier traces is shown by a characterisation of the noncommutative
integral in Connes' noncommutative geometry (for a wide class of Dixmier
traces) as a generalised limit of vector states associated to the eigenvectors
of a compact operator (or an unbounded operator with compact resolvent), i.e.
as a generalised quantum limit. Using the characterisation, a criteria
involving the eigenvectors of a compact operator and the projections of a von
Neumann subalgebra of bounded operators is given so that the noncommutative
integral associated to the compact operator is normal, i.e. satisfies a
monotone convergence theorem, for the von Neumann subalgebra.Comment: 15 page
GRB spectral parameter modeling
Fireball model of the gamma-ray bursts (GRBs) predicts generation of numerous
internal shocks, which efficiently accelerate charged particles and generate
relatively small-scale stochastic magnetic and electric fields. The accelerated
particles diffuse in space due to interaction with the random waves and so emit
so called Diffusive Synchrotron Radiation (DSR) in contrast to standard
synchrotron radiation they would produce in a large-scale regular magnetic
fields. In this contribution we present key results of detailed modeling of the
GRB spectral parameters, which demonstrate that the non-perturbative DSR
emission mechanism in a strong random magnetic field is consistent with
observed distributions of the Band parameters and also with cross-correlations
between them.Comment: 3 pages; IAU symposium # 274 "Advances in Plasma Astrophysics
Approximating acyclicity parameters of sparse hypergraphs
The notions of hypertree width and generalized hypertree width were
introduced by Gottlob, Leone, and Scarcello in order to extend the concept of
hypergraph acyclicity. These notions were further generalized by Grohe and
Marx, who introduced the fractional hypertree width of a hypergraph. All these
width parameters on hypergraphs are useful for extending tractability of many
problems in database theory and artificial intelligence. In this paper, we
study the approximability of (generalized, fractional) hyper treewidth of
sparse hypergraphs where the criterion of sparsity reflects the sparsity of
their incidence graphs. Our first step is to prove that the (generalized,
fractional) hypertree width of a hypergraph H is constant-factor sandwiched by
the treewidth of its incidence graph, when the incidence graph belongs to some
apex-minor-free graph class. This determines the combinatorial borderline above
which the notion of (generalized, fractional) hypertree width becomes
essentially more general than treewidth, justifying that way its functionality
as a hypergraph acyclicity measure. While for more general sparse families of
hypergraphs treewidth of incidence graphs and all hypertree width parameters
may differ arbitrarily, there are sparse families where a constant factor
approximation algorithm is possible. In particular, we give a constant factor
approximation polynomial time algorithm for (generalized, fractional) hypertree
width on hypergraphs whose incidence graphs belong to some H-minor-free graph
class
Searching for dark matter sterile neutrino in laboratory
If the dark matter of the Universe is made of sterile neutrinos with the mass
in keV region they can be searched for with the help of X-ray satellites. We
discuss the prospects of laboratory experiments that can be competitive and
complimentary to Space missions. We argue that the detailed study of beta
decays of tritium and other nuclei with the help of Cold Target Recoil Ion
Momentum Spectroscopy (COLTRIMS) can potentially enter into interesting
parameter range and even supersede the current astronomical bounds on the
properties of dark matter sterile neutrino.Comment: RevTex, 6 pages, 1 figure. Journal version accepted in Phys.Rev.
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