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1.
Within the framework of the conditions ; » –1 ( –1 is the mean time of momentum relaxation), the coefficient of absorption () of a weak electromagnetic wave by the free carriers of a polar semiconductor is calculated in the presence of a strong wave (of frequency ), for arbitrary values of and . Photon absorption by band electrons is due to these latter interacting with optical phonons (of frequency o). The problem is solved by using an analogous approach to the theory of the linear Kubo reaction. The results are valid in the absence of electron heating, when a strong wave only influences the scattering probability. The appearance of a photostimulated tail of absorption is predicted for < o, including the jump () for ( – o + ) 0T as well as peaks in the function () at the points s=s (s=1, 2, 3,...). The value (1) is determined by the formula for the absorption coefficient for one strong wave.Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 7, pp. 105–109, July, 1981.The authors are grateful to É. M. Épshtein and Sh. M. Kogan for useful discussions.  相似文献   

2.
For a bounded open domain with connected complement inR 2 and piecewise smooth boundary, we consider the Dirichlet Laplacian- on and the S-matrix on the complement c . We show that the on-shell S-matricesS k have eigenvalues converging to 1 askk 0 exactly when-- has an eigenvalue at energyk 0 2 . This includes multiplicities, and proves a weak form of transparency atk=k 0. We also show that stronger forms of transparency, such asS k 0 having an eigenvalue 1 are not expected to hold in general.  相似文献   

3.
The purpose of this paper is to review and to extend, wherever possible, the Kramers-Kronig relations, sum rules, and symmetry properties for the electrodynamic transport tensors of a linear plasma medium. For complete generality, we consider both nonrelativistic and relativistic plasmas with and without external magnetic fields. Our study is carried out first within the framework of classical electrodynamics. We then exploit the statistical-mechanical fluctuation-dissipation theorem to further obtain the Onsager symmetry relations and Kubo sum-rule frequency moments. Of special significance is the emergence of a variety of new Kramers-Kronig formulae andf-sum rules for the inverse dispersion tensor.Nomenclature E(k,) electric field intensity - Ê(k,) electric field in absence of plasma particles, - (k,) electric field due to the plasma particles (=E-Ê) - B(k,) magnetic induction - D(k,) electric induction - H(k,) magnetic field strength - B 0 constant external magnetic field - A 0 vector potential corresponding toB 0 - (k,),j(k, co) charge and current densities due to the plasma particles - (k,),J(k,) charge and current densities of the external agency - (k,,B 0) dielectric tensor of the plasma medium in the presence of B0 - (k,,B 0) diamagnetic tensor - (k, co,B 0) (k,,B 0) – 1, electric polarizability tensor - (k,,B 0) magnetic polarizability tensor - (k,,B 0) ordinary conductivity tensor - (k,,B 0) external conductivity tensor - D(k,,B 0) n2T–(k,,B 0), dispersion tensor, where T=1-kk is the transverse projection tensor (k being the unit vector in the direction ofk) andn = kc/ the index of refraction - n2T – 1, = vacuum wave operator (value of D in vacuum) - 1/2( + ), Hermitian part of - ^ 1/2( – ), Anti-Hermitian part of a - , real and imaginary parts of a - R(r,t) dissipated power per unit volume of plasma - U total energy absorbed by the plasma - R(k,) E*(k,) · (k,,b 0) ·E(k,) corresponding spectral energy density - W(r,t) 1/20E2(r, 0 + (l/20) B2(r,t), field energy density - W(k,) 1/20E*k,) ·E(k,) + (l/20)B *(k,) · B(k,), energy content in a certain domain of (k,)-space for a single mode - x i,p i,v i coordinate, momentum, and velocity of ith electron - i [1–(i 2/c2)]–1/2 - X j,P j,V j coordinate, momentum, and velocity of jth ion - {A q}, {Eq} field coordinates and momenta - jk(t),J k(t) perturbations in the microscopic electron and ion current densities due to the presence of the small external vector potential agencyâ(r,t) = (1/L3) âk(t) expi k ·r - Liouville distribution function = 0 + - 0 macrocanonical distribution function characterizing the equilibrium state of the system in the infinite past - small perturbation due toA - H0 Hamiltonian of equilibrium system which includes interaction - H Hamiltonian for the interaction between the system and the small external perturbing agencyA - 0 = dR()0 expectation value of any quantity over the equilibrium ensemble (dR is an element of hypervolume in -phase space) - G(12) two-particle distribution function - F(1) one-particle distribution function - g(¦x2 – x1 ¦) [G(12)/F(1)F(2)] – 1, pair correlation function - N total number of electron in volume L3 - n 0 equilibrium density (of electrons) - –1 temperature (in energy units) - 0 (n0e2/m0)1/2, equilibrium electron plasma frequency - c ¦e ¦–B 0/m, electron frequency - –1 ( 0/n0e2)1/2, Debye length - 0 (n0Ze2/M0)1/2, equilibrium ion plasma frequency - c ZeB0/M, ion cyclotron frequency  相似文献   

4.
In a previous paper asymptotic creation and annhilation operatorsa ± # have been constructed by the Kato-Mugibayashi method from the creation and annihilation operatorsa # for spin 1/2 fields with an interaction Hamiltonian density which is an evendegree polynomial in the field with ultra-violet cut-off and its derivatives. For any eigenvector of the total HamiltonianH=H 0+H I partial isometries ± have been defined so thata ± # equal ± a # *± on the ranges ± of ±. Since the existence of a groundstate ofH has been proved, the existence of at least one pair ± follows. The purpose of this paper is to show that for any ± orthogonal to the distribution of spins and momenta of the interacting Schrödinger states exp[–itH]± approaches fort the distributions of spins and momenta of the free state exp[–itH 0] if a wave-amplitude renormalization is carried out in ±. This is achieved by studying the expectation values of the operators in themaximally abelian W*-algebra generated by operators of the form a*a, in terms of whichany information about spins and momenta can be expressed.Supported in part by the National Research Council of Canada.  相似文献   

5.
A study is made of instability at frequencies close to the electron cyclotron frequency B and its multiples, subject to the presence of two different groups of electrons. It is shown that a mixture of hot and cold electrons ( ph 2 pc 2 ) in the region of frequencies s B, s2 can be unstable with respect to waves of the flute type (k z=0) with maximum increment max ( ph/pc). B, if there exists an interval of transversal velocities in whichF/ >0. When the curvature of the magnetic field is taken into account, even waves with B can be unstable in such a plasma. The effect of spatial inhomogeneity of the hot component on flute-type instability and on two-beam cyclotron instability is also examined.The author extends his thanks to A. B. Mikhajlovskij for his valuable comments and discussions.  相似文献   

6.
An expression is derived for the anomalous part (T, ) of the soft-mode damping function due to third-order interaction between critical optical phonons and acoustic phonons. It is shown that in crystals with a large elastic viscosity the damping function of critical phonons can have stronger temperature anomalies near phase-transition points. The frequency dispersion of () is investigated; it is found that the damping is a maximum at =o for the soft-mode vibrational dynamics and at =0 for the relaxational dynamics.Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 3, pp. 47–49, March, 1982.  相似文献   

7.
Evolution characters of angular velocity H of a Kerr black hole (BH) and distribution characters of angular velocity p of accreting particles near the BH horizon are investigated in the case of thin and thick disks, respectively. It is shown that H evolves in a non-monotonous way in the case of thin-disk-pure-accretion, attaining a maximum at a * 0.994. This evolution character turns out to depend on the radial gradient of p near the BH horizon. It is proved that both quantities, ( dH /dt) ms and ( p /r)r=r H, vanish at the same value of a *: a *0.994, and an explanation for the non-monotonousness of H is provided.  相似文献   

8.
Let (, , ) be a measure space with normalized measure,f: a nonsingular transformation. We prove: there exists anf-invariant normalized measure which is absolutely continuous with respect to if and only if there exist >0, and , 0<<1, such that (E)< implies (f –k(E))< for allk0.  相似文献   

9.
A class of the asymptotically Euclidian space-times is shown to exist for which the Schwarzschild mass is equal to zero. The coordinate atlases of these space-times satisfy two additional conditions: k (-gg 0k )=0 and ik 0 0g ik - ik k 0g 0i =0. In aT-orthogonal metricgs 2=g 00 dt 2 -g dx dx these conditions take a simple form: 0(detg )=0 and (0 g )(0 g )=0.  相似文献   

10.
Beginning with anLRC network with impedance functionZ(), a sequence of iterated networksN k with impedance functionsZ k(), k= 1, 2, 3,..., is introduced. The asymptotic comportment ofZ k() and the spectra ofN k are analyzed in terms of the Julia set ofZ. An example is given of an iterated network associated with a cascade of period-doubling bifurcations.  相似文献   

11.
Let be a von Neumann algebra with cyclic and separating vector , and letU(a) be a continuous unitary representation ofR with positive generator and as fixed point. If these unitaries induce for positive arguments endomorphisms of then the modular group act as dilatations on the group of unitaries. Using this it will be shown that every theory of local observables in two dimensions, which is covariant under translation only, can be imbedded into a theory of local observables covariant under the whole Poincaré group. This theory is also covariant under the CPT-transformation.  相似文献   

12.
It is demonstrated that for nondegenerate systems having a nonstationary nonlinearity the frequency condition k–1 + Re W(i) 0 (k < ) ensures exponential absolute stability.Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Radiofizika, Vol. 15, No. 3, pp. 319–322, March, 1972.  相似文献   

13.
A cold electron gas fills the lowest Landau level for high enough magnetic fields and for low enough densities. Such a situation is expected to occur for the Malmberg-O'Neil experiment and also for pulsar crusts and atmospheres. Such plasmas behave as a quasi-one-dimensional system and exhibit some peculiarities in their wave structure. We study the dispersion and damping of the low frequencies, i.e., the whistler mode, and the extraordinary mode for zero temperature. The behavior of the whistler mode depends critically on the filling number Fc=F/ , where F is the Fermi energy and is the cyclotron frequency. The one-dimensional character of the system affects the pair excitation spectrum and thus the decay of modes. We find that, in contrast to the three-dimensional situation, the plasma mode and the extraordinary mode remain undamped, while the whistler mode is undamped for all but very highk values.  相似文献   

14.
Starting axiomatically with a system of finite degrees of freedom whose logic c is an atomic Boolean -algebra, we prove the existence of phase space c, as a separable metric space, and a natural (weak) topology on the set of statesI (all the probability measures on c) such that c, the subspace of pure statesP, the set of atoms of c and the spaceP( c) of all the atomic measures on c, are all homeomorphic. The only physically accessible states are the points of c. This probabilistic formulation is shown to be reducible to a purely deterministic theory.  相似文献   

15.
This paper is concerned with a conjecture of Guillemin and Melrose that the length spectrum of a strictly convex bounded domain together with the spectra of the linear Poincaré maps corresponding to the periodic broken geodesics in determine uniquely the billiard ball map up to a symplectic conjugation. We consider continuous deformations of bounded domains s ,s[0, 1], with smooth boundaries and suppose that 0 is strictly convex and that the length spectrum does not change along the deformation. We prove that 0 is strictly convex for anys along the deformation and that for different values of the parameters the corresponding billiard ball maps are symplectically equivalent to each other on the union of the invariant KAM circles. We prove as well that the KAM circles and the restriction of the billiard ball map on them are spectral invariants of the Laplacian with Dirichlet (Neumann) boundary conditions for suitable deformations of strictly convex domains.Supported by Alexander von Humboldt foundation  相似文献   

16.
The problem of determining the total wave functions and energies of molecular stationary states reduces to solving a Schrödinger equation with a vibrational-rotational Hamiltonian. This is achieved by a unitary transformation of the molecular Hamiltonian H with its successive diagonalization on a nondegenerate electronic state ¦e. It is shown that the molecular wave functions related to the electronic states ¦e are of the form G¦e¦g(e), and their corresponding energy value is the sum e + g (e), where g (e) and ¦g(e) are the eigenvalues and eigenfunctions of the vibrational-rotational Hamiltonian, determined by means of the unitary operator G. It is shown that the total energy and molecular wave functions are uniquely determined, despite the arbitrariness in choosing G. As an example the vibrational-rotational operator and molecular wave functions are given for the simplest choice of the operator G.Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 3, pp. 11–16, March, 1975.  相似文献   

17.
We study a model in which a closed universe with dust and quintessence matter components may look like an accelerated flat Friedmann–Robertson–Walker (FRW) universe at low redshifts. Several quantities relevant to the model are expressed in terms of observed density parameters, M and , and of the associated density parameter Q related to the quintessence scalar field Q.  相似文献   

18.
In a recent note Barber showed, for a spin-1/2 Ising system with ferromagnetic pair interactions, that some critical exponents of the triplet order parameter i j k are the same as those of the magnetization i . Here we prove such results for all odd correlations and dispense with the requirement of pair interactions. We also prove that the critical temperatureT c , defined as the temperature below which there is a spontaneous magnetization, is for fixed even spin interactionsJ e independent of the way in which the odd interactionsJ o approach zero from above. This is achieved by using only the simplest, Griffiths-Kelley-Sherman (GKS), inequalities, which apply to the most general many-spin, ferromagnetic interactions.Research supported in part by NSF Grant #MPS 75-20638.  相似文献   

19.
In this paper, we study the spectrum of the Dirichlet Laplacian in a bounded (or, more generally, of finite volume) open set R n (n1) with fractal boundary of interior Minkowski dimension (n–1,n]. By means of the technique of tessellation of domains, we give the exact second term of the asymptotic expansion of the counting functionN() (i.e. the number of positive eigenvalues less than ) as +, which is of the form /2 times a negative, bounded and left-continuous function of . This explains the reason why the modified Weyl-Berry conjecture does not hold generally forn2. In addition, we also obtain explicit upper and lower bounds on the second term ofN().  相似文献   

20.
This paper presents results of an experimental investigation of fluctuations of intensity and arrival angle as a function of the parameter = ka2/L (where k = 2 /,a is the beam radius, and L is the length of the track) for tracks of different lengths. It is shown that, depending on the value of 0 2 = 1.23 C n 2 k7/6 L11/6, the intensity fluctuations can both increase, and also decrease with increase of . The fluctuations of arrival angle have a maximum for beams for which the parameter 5.Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, Vol. 16, No. 9, pp. 108–112, September, 1973.  相似文献   

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