Black Hole Evaporation as a Nonequilibrium Process ∗
... the number of independent helicities in radiation fields is N , the Stefan-Boltzmann constant becomes σ = N π 2 /120 (N = 2 for photon). Note that, due to the quasi-equilibrium assumption (Rg > O(1)), the NE model describes a semi-classical stage of evaporation, Tg < 1. Therefore it is appropriate t ...
... the number of independent helicities in radiation fields is N , the Stefan-Boltzmann constant becomes σ = N π 2 /120 (N = 2 for photon). Note that, due to the quasi-equilibrium assumption (Rg > O(1)), the NE model describes a semi-classical stage of evaporation, Tg < 1. Therefore it is appropriate t ...
Momentum
... of many particles is simply the vector sum of the individual momentum of each particle. • An isolated system is one in which the only forces present are those between the objects of the system. • It follows from Newton’s 3rd law that the total momentum of an isolated system of bodies remains constan ...
... of many particles is simply the vector sum of the individual momentum of each particle. • An isolated system is one in which the only forces present are those between the objects of the system. • It follows from Newton’s 3rd law that the total momentum of an isolated system of bodies remains constan ...
Correlated many-electron states in a quantum dot containing a
... take into account all states generated from the three specific quantum numbers: Ne, NS, and M 共here we take M = 5 / 2兲. Consequently, the Ne-electron quantum dot in the presence of the magnetic impurity has a Hamiltonian matrix that is six times larger than that in the case without the magnetic ion ...
... take into account all states generated from the three specific quantum numbers: Ne, NS, and M 共here we take M = 5 / 2兲. Consequently, the Ne-electron quantum dot in the presence of the magnetic impurity has a Hamiltonian matrix that is six times larger than that in the case without the magnetic ion ...
Establishing the Riemannian structure of space-time by
... The pseudo-Riemannian manifold of General Relativity is commonly accepted as the best mathematical model to describe space-time and the geometrized gravitation. A physical axiomatics of space-time should not postulate this particular geometrical structure from the beginning, but should make it a der ...
... The pseudo-Riemannian manifold of General Relativity is commonly accepted as the best mathematical model to describe space-time and the geometrized gravitation. A physical axiomatics of space-time should not postulate this particular geometrical structure from the beginning, but should make it a der ...
A Quantum Rosetta Stone for Interferometry
... difference between the two paths is then measured by balanced detection of the two output modes (see Fig. 1a). A similar situation, which we will omit in our discussion, can be found in Stern-Gerlach filters in series [23], and the technical limitations of such a device has been discussed by Englert ...
... difference between the two paths is then measured by balanced detection of the two output modes (see Fig. 1a). A similar situation, which we will omit in our discussion, can be found in Stern-Gerlach filters in series [23], and the technical limitations of such a device has been discussed by Englert ...
Advanced Quantum Mechanics - Pieter Kok
... where ¯ψ U and ¯φ V are typically not normalized (i.e., they are not unit vectors). The spaces U and V are so-called subspaces of W . As an example, consider the three-dimensional Euclidean space spanned by the Cartesian axes x, y, and z. The x y-plane is a two-dimensional subspace of the full space ...
... where ¯ψ U and ¯φ V are typically not normalized (i.e., they are not unit vectors). The spaces U and V are so-called subspaces of W . As an example, consider the three-dimensional Euclidean space spanned by the Cartesian axes x, y, and z. The x y-plane is a two-dimensional subspace of the full space ...
moment of inertia
... mass of the system and its angular counterpart is the so-called moment of inertia. The moment of inertia of a body is not only related to its mass but also the distribution of the mass throughout the body. So two bodies of the same mass may possess different moments of inertia. ...
... mass of the system and its angular counterpart is the so-called moment of inertia. The moment of inertia of a body is not only related to its mass but also the distribution of the mass throughout the body. So two bodies of the same mass may possess different moments of inertia. ...
