WEAK INTERACTION OF PHOTONS AND PROCESS GAMMA+GAMMA-]GAMMA+NU+NU

被引：5

作者：

CHAUDHURI, PR

机构：

[1] Electronics Division, Indian Statistical Institute, Calcutta

来源：

NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA A-NUCLEI PARTICLES AND FIELDS | 1969年 / 64卷 / 03期

关键词：

D O I：

10.1007/BF02721656

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

From the point of view that photons can interact weakly with neutrinos, the cross-section for the process π+π→π+ν+ ν - has been calculated. From this, the rate of stellar energy loss due to neutrino pair emission and neutrino luminosity of the star in this process has been calculated and the result is compared with that obtained on the basis of the current-current coupling theory. © 1969 Società Italiana di Fisica.

引用

页码：528 / +

页数：1

共 7 条

[1]

Akhiezer A.I., 1965, QUANTUM ELECTRODYNAM

[2] POSSIBLE WEAK INTERACTION OF PHOTONS AND EMISSION OF NEUTRINOS FROM STARS [J].

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PHYSICAL REVIEW, 1968, 173 (05) :1481-+

[3]

BANDYOPADHYAY P, TO BE PUBLISHED

[4] WEAK INTERACTION OF PHOTONS AND PHOTOCOULOMB NEUTRINOS [J].

CHAUDHURI, PR .

PROGRESS OF THEORETICAL PHYSICS, 1969, 42 (01) :116-+

[5]

CHAUDHURI PR, TO BE PUBLISHED

[6] ASTROPHYSICAL NEUTRINOS [J].

RUDERMAN, MA .

REPORTS ON PROGRESS IN PHYSICS, 1965, 28 :411-+

[7]

VANHIEU N, 1963, SOV PHYS JETP-USSR, V17, P681

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