Neutrino-electron elastic scattering and stellar energy loss through electron-positron pair annihilation in the magnetic model-Reference-Cited by-同舟云学术

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Neutrino-electron elastic scattering and stellar energy loss through electron-positron pair annihilation in the magnetic model

Published:1992-06 Issue:6 Volume:105 Page:843-849
ISSN:0369-3546
Container-title:Il Nuovo Cimento A
language:en
Short-container-title:Nuov Cim A

Author:

Aydin C.

Publisher

Springer Science and Business Media LLC

Subject

General Medicine

Link

http://link.springer.com/content/pdf/10.1007/BF02799099.pdf

Reference11 articles.

1. L. M. Brown:Phys. Today,31, 23 (1978).

2. E. Fermi:Z. Phys.,88, 161 (1934).

3. H. Bethe andC. I. Peierls:Nature,133, 532 (1934).

4. G. Gamow andM. Schönberg:Phys. Rev.,59, 534 (1941).

5. B. M. Pontecorvo:JETP,36, 1615 (1959).

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1. Role of neutrino form factors in the energy loss rates of the pair annihilation process;Chinese Physics C;2022-07-01

2. Stellar energy loss rates beyond the standard model;The European Physical Journal Plus;2020-06

3. $Z\to \nu\bar \nu\gamma$ DECAY IN BEYOND STANDARD MODEL;Modern Physics Letters A;2002-04-30

4. THE RATIOS OF ENERGY LOSSES THROUGH PHOTONEUTRINO PROCESS IN SUPERSTRING INSPIRED E6 MODEL AND IN THE STANDARD MODEL;Modern Physics Letters A;2001-03-14

5. THE PROCESSES $ e^+e^- \to \mu^+\mu^- ,\mu ^- \to e^- \bar{\nu}_e \nu_\mu ,\mu ^- \to e^- \gamma $ AND HEAVY NEUTRINO DECAY IN THE MAGNETIC MODEL;International Journal of Modern Physics A;1996-03-20

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