Neutrino Energy Loss in Stellar Interiors. VIII. Braaten-Segel Approximation for the Plasma Neutrino Process

The Astrophysical Journal ◽

10.1086/177926 ◽

1996 ◽

Vol 470 ◽

pp. 1015 ◽

Cited By ~ 26

Author(s):

Naoki Itoh ◽

Akinori Nishikawa ◽

Yasuharu Kohyama

Keyword(s):

Energy Loss ◽

Neutrino Energy ◽

Stellar Interiors

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Neutrino energy loss in stellar interiors. III - Pair, photo-, plasma, and bremsstrahlung processes

The Astrophysical Journal ◽

10.1086/167301 ◽

1989 ◽

Vol 339 ◽

pp. 354 ◽

Cited By ~ 143

Author(s):

Naoki Itoh ◽

Tomoo Adachi ◽

Masayuki Nakagawa ◽

Yasuharu Kohyama ◽

Hiroharu Munakata

Keyword(s):

Energy Loss ◽

Neutrino Energy ◽

Stellar Interiors

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Neutrino energy loss in stellar interiors. 6. Axial vector contribution to the plasma neutrino energy-loss rate for strongly degenerate electrons

The Astrophysical Journal ◽

10.1086/174527 ◽

1994 ◽

Vol 431 ◽

pp. 761 ◽

Cited By ~ 7

Author(s):

Yasuharu Kohyama ◽

Naoki Itoh ◽

Akihiko Obama ◽

Hiroshi Hayashi

Keyword(s):

Energy Loss ◽

Loss Rate ◽

Axial Vector ◽

Neutrino Energy ◽

Energy Loss Rate ◽

Stellar Interiors ◽

Strongly Degenerate

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Neutrino energy loss in stellar interiors. II - Axial-vector contribution to the plasma neutrino energy loss rate

The Astrophysical Journal ◽

10.1086/164734 ◽

1986 ◽

Vol 310 ◽

pp. 815 ◽

Cited By ~ 20

Author(s):

Yasuharu Kohyama ◽

Naoki Itoh ◽

Hiroharu Munakata

Keyword(s):

Energy Loss ◽

Loss Rate ◽

Axial Vector ◽

Neutrino Energy ◽

Energy Loss Rate ◽

Stellar Interiors

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Neutrino Energy Loss in Stellar Interiors. III. Pair, Photo-, Plasma, and Bremsstrahlung Processes: Erratum

The Astrophysical Journal ◽

10.1086/169160 ◽

1990 ◽

Vol 360 ◽

pp. 741 ◽

Cited By ~ 13

Author(s):

Itoh Naoki ◽

Tomoo Adachi ◽

Masayuki Nakagawa ◽

Yasuharu Kohyama ◽

Hiroharu Munakata

Keyword(s):

Energy Loss ◽

Neutrino Energy ◽

Stellar Interiors

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RADIATIVE CORRECTIONS TO NEUTRINO ENERGY LOSS RATE IN STELLAR INTERIORS

Modern Physics Letters A ◽

10.1142/s0217732302006643 ◽

2002 ◽

Vol 17 (08) ◽

pp. 491-502 ◽

Cited By ~ 10

Author(s):

S. ESPOSITO ◽

G. MANGANO ◽

G. MIELE ◽

I. PICARDI ◽

O. PISANTI

Keyword(s):

Energy Loss ◽

Loss Rate ◽

Neutrino Energy ◽

Tree Level ◽

Energy Loss Rate ◽

Star Evolution ◽

Cooling Mechanism ◽

Stellar Interiors ◽

Neutrino Pair ◽

Late Stages

We consider radiative electromagnetic corrections, at order α, to the process [Formula: see text] at finite density and temperature. This process represents one of the main contributions to the cooling of stellar environments in the late stages of star evolution. We find that these corrections affect the energy loss rate by a factor (-4-1)% with respect to the tree level estimate, in the temperature and density ranges where the neutrino pair production via e+e- annihilation is the most efficient cooling mechanism.

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