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2003 | 1 | 1 | 145-152
Tytuł artykułu

Energy and momentum losses in the process of neutrino scattering on plasma electrons in the presence of a magnetic field

Treść / Zawartość
Warianty tytułu
Języki publikacji
EN
Abstrakty
EN
The neutrino-electron scattering in a dense degenerate magnetized plasma under the conditions μ 2 > 2eB ≫ μE is investigated. The volume density of the neutrino energy and momentum losses due to this process are calculated. The results we have obtained demonstrate that plasma in the presence of an external magnetic field is more transparent for neutrino than for non-magnetized plasma. It is shown that neutrino scattering under conditions considered does not lead to the neutrino force acting on plasma.
Wydawca

Czasopismo
Rocznik
Tom
1
Numer
1
Strony
145-152
Opis fizyczny
Daty
wydano
2003-03-01
online
2003-03-01
Twórcy
  • Division of Theoretical Physics, Department of Physics, Yaroslavl State University, Sovietskaya 14, 150000, Yaroslavl, Russian Federation, mikheev@univ.uniyar.ac.ru
  • Division of Theoretical Physics, Department of Physics, Yaroslavl State University, Sovietskaya 14, 150000, Yaroslavl, Russian Federation, elenan@univ.uniyar.ac.ru
Bibliografia
  • [1] Bezchastnov, V.G. and Haensel, P. 1996. Neutrino-electron scattering in a dense magnetized plasma. Physical Review D, 54 (6), 3706–371. http://dx.doi.org/10.1103/PhysRevD.54.3706[Crossref]
  • [2] Bisnovatyi-Kogan, G.S., 1993. Physical Problems of Theory of Stellar Evolution. Nauka: Moscow
  • [3] Duncan, R.C. and Thompson, C. 1992. Formation of very strongly magnetized neutron stars: implications for gamma-ray bursts. Astrophysical Journal, 392, L9–L13. http://dx.doi.org/10.1086/186413[Crossref]
  • [4] Gvozdev, A.A. and Ognev, I.S. 1999. On the possible enhancement of the magnetic field by neutrino re-emission processes in the mantle of a supernova. JETP Letters, 69 (5), 365–370. http://dx.doi.org/10.1134/1.568035[Crossref]
  • [5] Kuznetsov, A.V. and Mikheev, N.V., 2000. Neutrino interaction with strongly magnetized electron-positron plasma. Journal of Experimental and Theoretical Physics, 91 (4), 748–760. http://dx.doi.org/10.1134/1.1326967[Crossref]
  • [6] Mathews, G.J. et al., 1997. Gamma-ray bursts from neutron star binaries. Preprint astroph/9710229.
  • [7] Mezzacappa, A. and Bruenn, S.W., 1993. Stellar core collapse: a Boltzmann treatment of neutrino-electron scattering. Astrophysical Journal, 410, 740–760. http://dx.doi.org/10.1086/172791[Crossref]
  • [8] Mikheev, N.V. and Narynskaya, E.N., 2000. Neutrino-electron processes in a dense magnetized plasma. Modern Physics Letters A, 15 (25), 1551–1556. http://dx.doi.org/10.1016/S0217-7323(00)00200-0[Crossref]
  • [9] Raffelt, G.G., 1996. Stars as Laboratories for Fundamental Physics, University of Chicago Press: Chicago.
Typ dokumentu
Bibliografia
Identyfikatory
Identyfikator YADDA
bwmeta1.element.-psjd-doi-10_2478_BF02475558
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