首页 | 本学科首页   官方微博 | 高级检索  
相似文献
 共查询到20条相似文献,搜索用时 15 毫秒
1.
Let (M,g)(M,g) be a noncompact complete Bach-flat manifold with positive Yamabe constant. We prove that (M,g)(M,g) is flat if (M,g)(M,g) has zero scalar curvature and sufficiently small L2L2 bound of curvature tensor. When (M,g)(M,g) has nonconstant scalar curvature, we prove that (M,g)(M,g) is conformal to the flat space if (M,g)(M,g) has sufficiently small L2L2 bound of curvature tensor and L4/3L4/3 bound of scalar curvature.  相似文献   

2.
Let MM be a connected compact quantizable Kähler manifold equipped with a Hamiltonian action of a connected compact Lie group GG. Let M//G=?−1(0)/G=M0M//G=?1(0)/G=M0 be the symplectic quotient at value 0 of the moment map ??. The space M0M0 may in general not be smooth. It is known that, as vector spaces, there is a natural isomorphism between the quantum Hilbert space over M0M0 and the GG-invariant subspace of the quantum Hilbert space over MM. In this paper, without any regularity assumption on the quotient M0M0, we discuss the relation between the inner products of these two quantum Hilbert spaces under the above natural isomorphism; we establish asymptotic unitarity to leading order in Planck’s constant of a modified map of the above isomorphism under a “metaplectic correction” of the two quantum Hilbert spaces.  相似文献   

3.
We discuss three different ways to arrive at kaon condensation at nc?3n0nc?3n0 where n0n0 is nuclear matter density: (1) Fluctuating around the n=0n=0 vacuum in chiral perturbation theory, (2) fluctuating around nVMnVM near the chiral restoration density nχnχ where the vector manifestation of hidden local symmetry is reached and (3) fluctuating around the Fermi liquid fixed point at ∼n0n0. They all share one common theoretical basis, “hidden local symmetry”. We argue that when the critical density nc<nχnc<nχ is reached in a neutron star, the electrons turn into KK mesons, which go into an s-wave Bose condensate. This reduces the pressure substantially and the neutron star goes into a black hole. Next we develop the argument that the collapse of a neutron star into a black hole takes place for a star of M?1.5MM?1.5M. This means that Supernova 1987A had a black hole as result. We also show that two neutron stars in a binary have to be within 4% of each other in mass, for neutron stars sufficiently massive that they escape helium shell burning. For those that are so light that they do have helium shell burning, after a small correction for this, they must be within 4% of each other in mass. Observations support the proximity in mass inside of a neutron star binary. The result of strangeness condensation is that there are ∼55 times more low-mass black-hole, neutron-star binaries than double neutron-star binaries although the former are difficult to observe.  相似文献   

4.
We study reduction of generalized complex structures. More precisely, we investigate the following question. Let JJ be a generalized complex structure on a manifold MM, which admits an action of a Lie group GG preserving JJ. Assume that M0M0 is a GG-invariant smooth submanifold and the GG-action on M0M0 is proper and free so that MG?M0/GMG?M0/G is a smooth manifold. Under what condition does JJ descend to a generalized complex structure on MGMG? We describe a sufficient condition for the reduction to hold, which includes the Marsden–Weinstein reduction of symplectic manifolds and the reduction of the complex structures in Kähler manifolds as special cases. As an application, we study reduction of generalized Kähler manifolds.  相似文献   

5.
We demonstrate the emergence of non-Abelian fusion rules for excitations of a two dimensional lattice model built out of Abelian degrees of freedom. It can be considered as an extension of the usual toric code model on a two dimensional lattice augmented with matter fields. It consists of the usual C(Zp)C(Zp) gauge degrees of freedom living on the links together with matter degrees of freedom living on the vertices. The matter part is described by a nn dimensional vector space which we call HnHn. The ZpZp gauge particles act on the vertex particles and thus HnHn can be thought of as a C(Zp)C(Zp) module. An exactly solvable model is built with operators acting in this Hilbert space. The vertex excitations for this model are studied and shown to obey non-Abelian fusion rules. We will show this for specific values of nn and pp, though we believe this feature holds for all n>pn>p. We will see that non-Abelian anyons of the quantum double of C(S3)C(S3) are obtained as part of the vertex excitations of the model with n=6n=6 and p=3p=3. Ising anyons are obtained in the model with n=4n=4 and p=2p=2. The n=3n=3 and p=2p=2 case is also worked out as this is the simplest model exhibiting non-Abelian fusion rules. Another common feature shared by these models is that the ground states have a higher symmetry than ZpZp. This makes them possible candidates for realizing quantum computation.  相似文献   

6.
Geometrical characterizations are given for the tensor R⋅SRS, where SS is the Ricci tensor   of a (semi-)Riemannian manifold (M,g)(M,g) and RR denotes the curvature operator   acting on SS as a derivation, and of the Ricci Tachibana tensor  g⋅SgS, where the natural metrical operator  gg also acts as a derivation on SS. As a combination, the Ricci curvatures   associated with directions on MM, of which the isotropy determines that MM is Einstein, are extended to the Ricci curvatures of Deszcz   associated with directions and planes on MM, and of which the isotropy determines that MM is Ricci pseudo-symmetric in the sense of Deszcz.  相似文献   

7.
We address the question of thermodynamical evolution of regular spherically symmetric cosmological black holes with de Sitter center. Space–time is asymptotically de Sitter as r→0r0 and as r→∞r. A source term in the Einstein equations connects smoothly two de Sitter vacua with different values of cosmological constant and corresponds to anisotropic vacuum dark fluid defined by symmetry of its stress–energy tensor. In the range of masses Mcr1?M?Mcr2Mcr1?M?Mcr2 it describes a regular cosmological black hole with three horizons, an internal horizon rara, a black hole horizon rb>rarb>ra, and a cosmological horizon rc>rbrc>rb. Thermodynamical preference for a final product of evaporation is a double-horizon (ra=rbra=rb) black hole remnant with the positive specific heat.  相似文献   

8.
Let MM be a connected complex projective manifold such that c1(T(1,0)M)=0c1(T(1,0)M)=0. If MM admits a holomorphic Cartan geometry, then we show that MM is holomorphically covered by an abelian variety.  相似文献   

9.
We construct a natural L2L2-metric on the perturbed Seiberg–Witten moduli spaces Mμ+Mμ+ of a compact 4-manifold MM, and we study the resulting Riemannian geometry of Mμ+Mμ+. We derive a formula which expresses the sectional curvature of Mμ+Mμ+ in terms of the Green operators of the deformation complex of the Seiberg–Witten equations. In case MM is simply connected, we construct a Riemannian metric on the Seiberg–Witten principal U(1)U(1) bundle P→Mμ+PMμ+ such that the bundle projection becomes a Riemannian submersion. On a Kähler surface MM, the L2L2-metric on Mμ+Mμ+ coincides with the natural Kähler metric on moduli spaces of vortices.  相似文献   

10.
We consider the possibility that the soft supersymmetry-breaking parameters m1/2m1/2 and m0m0 of the MSSM are universal at some scale MinMin below the supersymmetric grand unification scale MGUTMGUT, as might occur in scenarios where either the primordial supersymmetry-breaking mechanism or its communication to the observable sector involve a dynamical scale below MGUTMGUT. We analyze the (m1/2,m0)(m1/2,m0) planes of such sub-GUT CMSSM models, noting the dependences of phenomenological, experimental and cosmological constraints on MinMin. In particular, we find that the coannihilation, focus-point and rapid-annihilation funnel regions of the GUT-scale CMSSM approach and merge when Min∼1012 GeVMin1012 GeV. We discuss sparticle spectra and the possible sensitivity of LHC measurements to the value of MinMin.  相似文献   

11.
A family of spherically symmetric solutions with horizon in the model with m  -component anisotropic fluid is presented. The metrics are defined on a manifold that contains a product of n−1n1 Ricci-flat “internal” spaces. The equation of state for any s  -th component is defined by a vector UsUs belonging to Rn+1Rn+1. The solutions are governed by moduli functions HsHs obeying non-linear differential equations with certain boundary conditions imposed. A simulation of black brane solutions in the model with antisymmetric forms is considered. An example of solution imitating M2–M5M2M5 configuration (in D=11D=11 supergravity) corresponding to Lie algebra A2A2 is presented.  相似文献   

12.
Amovilli and March (2006) [8] used diffusion quantum Monte Carlo techniques to calculate the non-relativistic ionization potential I(Z)I(Z) in He-like atomic ions for the range of (fractional) nuclear charges Z   lying between the known critical value Zc=0.911Zc=0.911 at which I(Z)I(Z) tends to zero and Z=2Z=2. They showed that it is possible to fit I(Z)I(Z) to a simple quadratic expression. Following that idea, we present here a semiempirical fine-tuning of Hartree–Fock ionization potentials for the isoelectronic series of He, Be, Ne, Mg and Ar-like atomic ions that leads to excellent estimations of ZcZc for these series. The empirical information involved is experimental ionization and electron affinity data. It is clearly demonstrated that Hartree–Fock theory provides an excellent starting point for determining I(Z)I(Z) for these series.  相似文献   

13.
We calculate low scale gravity effects on the cross section for neutrino–nucleon scattering at center of mass energies up to the Greisen–Zatsepin–Kuzmin (GZK) scale, in the eikonal approximation. We compare the cases of an infinitely thin brane embedded in n=5n=5 compactified extra-dimensions, and of a brane with a physical tension MS=1 TeVMS=1 TeV and MS=10 TeVMS=10 TeV. The extra dimensional Planck scale MDMD is set at 103 GeV103 GeV and 2×103 GeV2×103 GeV. We also compare our calculations with neutral current standard model calculations in the same energy range, and compare the thin brane eikonal cross section to its saddle point approximation. New physics effects enhance the cross section by orders of magnitude on average. They are quite sensitive to MSMS and MDMD choices, though much less sensitive to n.  相似文献   

14.
We discuss three Hamiltonians, each with a central-field part H0H0 and a PT-symmetric perturbation igzigz. When H0H0 is the isotropic Harmonic oscillator the spectrum is real for all gg because HH is isospectral to H0+g2/2H0+g2/2. When H0H0 is the Hydrogen atom then infinitely many eigenvalues are complex for all gg. If the potential in H0H0 is linear in the radial variable rr then the spectrum of HH exhibits real eigenvalues for 0<g<gc0<g<gc and a PT phase transition at gcgc.  相似文献   

15.
We consider a Schrödinger differential expression L=ΔA+qL=ΔA+q on a complete Riemannian manifold (M,g)(M,g) with metric gg, where ΔAΔA is the magnetic Laplacian on MM and q≥0q0 is a locally square integrable function on MM. In the terminology of W.N. Everitt and M. Giertz, the differential expression LL is said to be separated in L2(M)L2(M) if for all u∈L2(M)uL2(M) such that Lu∈L2(M)LuL2(M), we have qu∈L2(M)quL2(M). We give sufficient conditions for LL to be separated in L2(M)L2(M).  相似文献   

16.
Current experimental data indicate that two unitarity triangles of the CKM quark mixing matrix V   are almost the right triangles with α≈90°α90°. We highlight a very suggestive parametrization of V and show that its CP-violating phase ? is nearly equal to α   (i.e., ?−α≈1.1°?α1.1°). Both ? and α   are stable against the renormalizaton-group evolution from the electroweak scale MZMZ to a superhigh energy scale MXMX or vice versa, and thus it is impossible to obtain α=90°α=90° at MZMZ from ?=90°?=90° at MXMX. We conjecture that there might also exist a maximal CP-violating phase φ≈90°φ90° in the MNS lepton mixing matrix U. The approximate quark–lepton complementarity relations, which hold in the standard parametrizations of V and U, can also hold in our particular parametrizations of V and U   simply due to the smallness of |Vub||Vub| and |Ve3||Ve3|.  相似文献   

17.
We have studied the anisotropic two-dimensional nearest-neighbor Ising model with competitive interactions in both uniform longitudinal field HH and transverse magnetic field ΩΩ. Using the effective-field theory (EFT) with correlation in cluster with N=1N=1 spin we calculate the thermodynamic properties as a function of temperature with values HH and ΩΩ fixed. The model consists of ferromagnetic interaction JxJx in the xx direction and antiferromagnetic interaction JyJy in the yy direction, and it is found that for H/Jy∈[0,2]H/Jy[0,2] the system exhibits a second-order phase transition. The thermodynamic properties are obtained for the particular case of λ=Jx/Jy=1λ=Jx/Jy=1 (isotropic square lattice).  相似文献   

18.
In order to explain the occurrence of a minimum in firing rate which occurs for certain mean input levels μμ as noise level σσ increases (inverse stochastic resonance, ISR) in Hodgkin–Huxley (HH) systems, we analyze the underlying transitions from a stable equilibrium point to limit cycle and vice-versa. For a value of μμ at which ISR is pronounced, properties of the corresponding stable equilibrium point are found. A linearized approximation around this point has oscillatory solutions from whose maxima spikes tend to occur. A one dimensional diffusion is also constructed for small noise. Properties of the basin of attraction of the limit cycle (spike) are investigated heuristically. Long term trials of duration 500000 ms are carried out for values of σσ from 0 to 2.0. The graph of mean spike count versus σσ is divided into 4 regions R1,…,R4R1,,R4, where R3R3 contains the minimum associated with ISR. In R1R1 transitions to the basin of attraction of the rest point are not observed until a small critical value of σ=σc1σ=σc1 is reached, at the beginning of R2R2. The sudden decline in firing rate when σσ is just greater than σc1σc1 implies that there is only a small range of noise levels 0<σ<σc10<σ<σc1 where repetitive spiking is safe from annihilation by noise. The firing rate remains small throughout R3R3. At a larger critical value σ=σc2σ=σc2 which signals the beginning of R4R4, the probability of transitions from the basin of attraction of the equilibrium point to that of the limit cycle apparently becomes greater than zero and the spike rate thereafter increases with increasing σσ. The quantitative scheme underlying the ISR curve is outlined in terms of the properties of exit time random variables. In the final subsection, several statistical properties of the main random variables associated with long term spiking activity are given, including distributions of exit times from the two relevant basins of attraction and the interspike interval.  相似文献   

19.
20.
We analyse the phase diagram of a quantum mean spherical model in terms of the temperature TT, a quantum parameter gg, and the ratio p=−J2/J1p=J2/J1, where J1>0J1>0 refers to ferromagnetic interactions between first-neighbour sites along the dd directions of a hypercubic lattice, and J2<0J2<0 is associated with competing antiferromagnetic interactions between second neighbours along m≤dmd directions. We regain a number of known results for the classical version of this model, including the topology of the critical line in the g=0g=0 space, with a Lifshitz point at p=1/4p=1/4, for d>2d>2, and closed-form expressions for the decay of the pair correlations in one dimension. In the T=0T=0 phase diagram, there is a critical border, gc=gc(p)gc=gc(p) for d≥2d2, with a singularity at the Lifshitz point if d<(m+4)/2d<(m+4)/2. We also establish upper and lower critical dimensions, and analyse the quantum critical behavior in the neighborhood of p=1/4p=1/4.  相似文献   

设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号