34,362 research outputs found

    Incompressibility of orthogonal grassmannians

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    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

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    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 \ellth-order empirical entropy stops being a reasonable complexity metric for almost all strings of length mm over alphabets of size nn about when nn^\ell surpasses mm

    The Compression-Mode Giant Resonances and Nuclear Incompressibility

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    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

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    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 a1a_1 and the symmetry energy JJ are around the acceptable values 16MeV and 30MeV respectively; the incompressibility K0K_0 is unacceptably high in the linear model, but assumes reasonable value if nonlinear terms are included; the density symmetry LL is around 100MeV100MeV for most parameter sets, and the symmetry incompressibility KsK_s has positive sign which is opposite to expectations based on the nonrelativistic model. In almost all parameter sets there exists a critical point (ρc,δc)(\rho_c, \delta_c), where the minimum and the maximum of the equation of state are coincident and the incompressibility equals zero, falling into ranges 0.014fm3<ρc<0.039^{-3}<\rho_c<0.039fm3^{-3} and 0.74<δc0.950.74<\delta_c\le0.95; for a few parameter sets there is no critical point and the pure neutron matter is predicted to be bound. The maximum mass MNSM_{NS} of neutron stars is predicted in the range 2.45MMNS3.26_\odot\leq M_{NS}\leq 3.26M_\odot, the corresponding neutron star radius RNSR_{NS} is in the range 12.2kmRNS15.1\leq R_{NS}\leq 15.1km.Comment: 10 pages, 5 figure

    Incompressibility Estimates for the Laughlin Phase

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    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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