Optical Orientation in Strained Semiconductors

Dzhioev, R. I.; Fleischer, Viktoriya; Ivchenko, E. L.; Vecua, V. L.; Zakharchenya, B. P.

doi:10.1007/978-3-322-94774-1_132

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2014

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Cited by 3 publications

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“…In the most practical cases one cannot diagonalize H exactly. Let us assume that we diagonalize the thermal nuclear Hamiltonian by invoking some approximation methods (e.g., 2 The correspondence between the thermo field dynamics and the superoperator formalism used one of the authors (A.D.) to study nonequilibrium electron transport phenomena (see, e.g., [14]) is discussed in [15].…”

Section: Formalismmentioning

confidence: 99%

Neutrino-antineutrino pair emission from thermally excited nuclei in stellar collapse

Dzhioev¹,

Vdovin²

2014

Phys. Atom. Nuclei

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We examine the rate of neutrino-antineutrino pair emission by hot nuclei in collapsing stellar cores. The rates are calculated assuming that only allowed charge-neutral Gamow-Teller (GT 0 ) transitions contribute to the decay of thermally excited nuclear states. To obtain the GT 0 transition matrix elements, we employ the quasiparticle random phase approximation extended to finite temperatures within the thermo field dynamics formalism. The decay rates and the energy emission rates are calculated for the sample nuclei 56 Fe and 82 Ge at temperatures relevant to core collapse supernovae.

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Section: Formalismmentioning

confidence: 99%