34,362 research outputs found
Incompressibility of orthogonal grassmannians
We prove the following conjecture due to Bryant Mathews (2008). Let Q be the
orthogonal grassmannian of totally isotropic i-planes of a non-degenerate
quadratic form q over an arbitrary field (where i is an integer in the interval
[1, (\dim q)/2]). If the degree of each closed point on Q is divisible by 2^i
and the Witt index of q over the function field of Q is equal to i, then the
variety Q is 2-incompressible.Comment: 5 page
Large Alphabets and Incompressibility
We briefly survey some concepts related to empirical entropy -- normal
numbers, de Bruijn sequences and Markov processes -- and investigate how well
it approximates Kolmogorov complexity. Our results suggest th-order
empirical entropy stops being a reasonable complexity metric for almost all
strings of length over alphabets of size about when surpasses
The Compression-Mode Giant Resonances and Nuclear Incompressibility
The compression-mode giant resonances, namely the isoscalar giant monopole
and isoscalar giant dipole modes, are examples of collective nuclear motion.
Their main interest stems from the fact that one hopes to extrapolate from
their properties the incompressibility of uniform nuclear matter, which is a
key parameter of the nuclear Equation of State (EoS). Our understanding of
these issues has undergone two major jumps, one in the late 1970s when the
Isoscalar Giant Monopole Resonance (ISGMR) was experimentally identified, and
another around the turn of the millennium since when theory has been able to
start giving reliable error bars to the incompressibility. However, mainly
magic nuclei have been involved in the deduction of the incompressibility from
the vibrations of finite nuclei. The present review deals with the developments
beyond all this. Experimental techniques have been improved, and new
open-shell, and deformed, nuclei have been investigated. The associated changes
in our understanding of the problem of the nuclear incompressibility are
discussed. New theoretical models, decay measurements, and the search for the
evolution of compressional modes in exotic nuclei are also discussed.Comment: Review paper to appear in "Progress in Particle and Nuclear Physics
Nuclear matter properties and relativistic mean-field theory
Nuclear matter properties are calculated in the relativistic mean field
theory by using a number of different parameter sets. The result shows that the
volume energy and the symmetry energy are around the acceptable
values 16MeV and 30MeV respectively; the incompressibility is
unacceptably high in the linear model, but assumes reasonable value if
nonlinear terms are included; the density symmetry is around for
most parameter sets, and the symmetry incompressibility has positive sign
which is opposite to expectations based on the nonrelativistic model. In almost
all parameter sets there exists a critical point , where
the minimum and the maximum of the equation of state are coincident and the
incompressibility equals zero, falling into ranges
0.014fmfm and ; for a few
parameter sets there is no critical point and the pure neutron matter is
predicted to be bound. The maximum mass of neutron stars is predicted
in the range 2.45MM, the corresponding
neutron star radius is in the range 12.2kmkm.Comment: 10 pages, 5 figure
Incompressibility Estimates for the Laughlin Phase
This paper has its motivation in the study of the Fractional Quantum Hall
Effect. We consider 2D quantum particles submitted to a strong perpendicular
magnetic field, reducing admissible wave functions to those of the Lowest
Landau Level. When repulsive interactions are strong enough in this model,
highly correlated states emerge, built on Laughlin's famous wave function. We
investigate a model for the response of such strongly correlated ground states
to variations of an external potential. This leads to a family of variational
problems of a new type. Our main results are rigorous energy estimates
demonstrating a strong rigidity of the response of strongly correlated states
to the external potential. In particular we obtain estimates indicating that
there is a universal bound on the maximum local density of these states in the
limit of large particle number. We refer to these as incompressibility
estimates
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