1,341 research outputs found
Attenuation of super-soft X-ray sources by circumstellar material
Recent studies have suggested the possibility of significantly obscuring
super-soft X-ray sources in relatively modest amounts of local matter lost from
the binaries themselves. If correct, then this would have explained the paucity
of observed super-soft X-ray sources and would have significance for the search
for single-degenerate type Ia supernova progenitors. We point out that earlier
studies of circumbinary obscuration ignored photo-ionisations of the gas by the
emission from the super-soft X-ray source. We revisit the problem using a full,
self-consistent calculation of the ionisation state of the circumbinary
material photo-ionised by the radiation of the central source. Our results show
that the circumstellar mass-loss rates required for obcuration of super-soft
X-ray sources is about an order of magnitude larger than those reported in
earlier studies, for comparable model parameters. While this does not entrirely
rule out the possibility of circumstellar material obscuring super-soft X-ray
sources, it makes it unlikely that this effect alone can account for the
majority of the missing super-soft X-ray sources. We discuss the observational
appearance of hypothetical obscured nuclear burning white dwarfs and show that
they have signatures making them distinct from photo-ionised nebulae around
super-soft X-ray sources imbedded in the low density ISM.Comment: MNRAS, accepted; 11 pages, 10 figures, 1 tabl
Non-Commutative Open (p,q)-String Theories
In this paper we make an SL(2,Z)-covariant generalisation of the
noncommutative theories, NCYM and NCOS on the D3-brane, and NCOS on the
D5-brane in type IIB. Usually, the noncommutative theories are obtained by
studying perturbative F-string theory, and the parameters governing the
noncommutative theories are given by the open string data. The S-duality of
NCYM and NCOS on the D3-brane has been seen by dualising the background,
keeping the F-string under study fixed. We give an SL(2,Z)-covariant
generalisation of the open string data relevant when one instead studies
perturbative (p,q)-string theory. The S-duality of NCYM and NCOS on the
D3-brane is reproduced by instead keeping the background fixed and studying
different (p,q)-string theories. We also obtain new noncommutative open
(p,q)-string theories on the D3-brane and the D5-brane which are S-dual to
ordinary NCOS. The theories are studied using the supergravity duals of the
D3-brane and the D5-brane, corresponding to a probe brane in the relevant
background.Comment: AMSLaTeX. 23 pages. Minor clarifications added. To be published in
JHE
Hardness of Bichromatic Closest Pair with Jaccard Similarity
Consider collections and of red and blue sets,
respectively. Bichromatic Closest Pair is the problem of finding a pair from
that has similarity higher than a given
threshold according to some similarity measure. Our focus here is the classic
Jaccard similarity
for .
We consider the approximate version of the problem where we are given
thresholds and wish to return a pair from that has Jaccard similarity higher than if there exists a
pair in with Jaccard similarity at least .
The classic locality sensitive hashing (LSH) algorithm of Indyk and Motwani
(STOC '98), instantiated with the MinHash LSH function of Broder et al., solves
this problem in time if . In
particular, for , the approximation ratio
increases polynomially in .
In this paper we give a corresponding hardness result. Assuming the
Orthogonal Vectors Conjecture (OVC), we show that there cannot be a general
solution that solves the Bichromatic Closest Pair problem in
time for . Specifically, assuming
OVC, we prove that for any there exists an such that
Bichromatic Closest Pair with Jaccard similarity requires time
for any choice of thresholds , that
satisfy
Obscuring Supersoft X-ray Sources in Stellar Winds
We investigate the possibility of obscuring supersoft X-ray sources in the
winds of companion stars. We derive limits on the amount of circumstellar
material needed to fully obscure a 'canonical' supersoft X-ray source in the
Large Magellanic Cloud, as observed with the Chandra X-ray Observatory.Comment: Conference proceedings for IAU Symposium no. 281 "Binary Paths to
Type Ia Supernova Explosions", 5-10 July 2011, Padova, Ital
Architecture and noise analysis of continuous variable quantum gates using two-dimensional cluster states
Due to its unique scalability potential, continuous variable quantum optics
is a promising platform for large scale quantum computing and quantum
simulation. In particular, very large cluster states with a two-dimensional
topology that are suitable for universal quantum computing and quantum
simulation can be readily generated in a deterministic manner, and routes
towards fault-tolerance via bosonic quantum error-correction are known. In this
article we propose a complete measurement-based quantum computing architecture
for the implementation of a universal set of gates on the recently generated
two-dimensional cluster states [1,2]. We analyze the performance of the various
quantum gates that are executed in these cluster states as well as in other
two-dimensional cluster states (the bilayer-square lattice and quad-rail
lattice cluster states [3,4]) by estimating and minimizing the associated
stochastic noise addition as well as the resulting gate error probability. We
compare the four different states and find that, although they all allow for
universal computation, the quad-rail lattice cluster state performs better than
the other three states which all exhibit similar performance
- …