11,076 research outputs found
Slow scrambling in sonic black holes
We study from the perspective of quantum information scrambling an acoustic
black hole modelled by two semi-infinite, stationary, one dimensional
condensates, connected by a spatial step-like discontinuity, and flowing
respectively at subsonic and supersonic velocities. We develop a simple
analytical treatment based on Bogolyubov theory of quantum fluctuations which
is sufficient to derive analogue Hawking emission, and we compute out-of-time
order correlations (OTOCs) of the Bose density field. We find that sonic black
holes are slow scramblers contrary to their astrophysical counterparts: this
manifests in a power law growth of OTOCs in contrast to the
exponential increase in time expected for fast scramblers.Comment: 5 pages, 2 figure
Quark matter equation of state and stellar properties
In this paper we study strange matter by investigating the stability window
within the QMDD model at zero temperature and check that it can explain the
very massive pulsar recently detected. We compare our results with the ones
obtained from the MIT bag model and see that the QMDD model can explain larger
masses, due to the stiffening of the equation of state
Coasian Dynamics in Repeated English Auctions
We extend the Coase conjecture to the case of a seller with a single object, who faces n potential buyers and holds a sequence of English auctions until the object is sold. In an independent-private-values environment in which buyers and sellers share the same discount factor, we show that the (perfect Bayesian) equilibrium path of reserve prices obeys a Coasian logic. Moreover, the equilibrium reserve path lies below that for the model of repeated sealed-bid, second-price auctions studied by McAfee and Vincent (1997). Nevertheless, the open (English) and sealed-bid formats are shown to be revenue equivalent.
Evolution of the fine-structure constant in the non-linear regime
We study the evolution of the fine-structure constant, , induced by
non-linear density perturbations in the context of the simplest class of
quintessence models with a non-minimal coupling to the electromagnetic field,
in which the two available free functions (potential and gauge kinetic
function) are Taylor-expanded up to linear order. We show that the results
obtained using the spherical infall model for an infinite wavelength
inhomogeneity are inconsistent with the results of a local linearized gravity
study and we argue in favour of the second approach. We also discuss recent
claims that the value of inside virialised regions could be
significantly different from the background one on the basis of these findings.Comment: 5 pages, 3 figure
Stability windows for proto-quark stars
We investigate the existence of possible stable strange matter and related
stability windows at finite temperature for different models that are generally
applied to describe quark stars, namely, the quark-mass density dependent
model, the MIT bag model and the Nambu-Jona-Lasinio model. We emphasize that,
although the limits for stable strange matter depend on a comparison with the
ground state of 56Fe, which is a zero temperature state, the quantity that has
to be used in the search for strange matter in proto-quark stars is the free
energy and we analyze stability windows up to temperatures of the order of 40
MeV. The effects of strong magnetic fields on stability windows are computed
and the resulting mass-radius relations for different stages of the proto-quark
star are analyzed.Comment: Published versio
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