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Volumn 70, Issue 4, 2004, Pages

SN1987A and the properties of the neutrino burst

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; ASTRONOMY; ELECTRON; ENERGY; MATHEMATICAL ANALYSIS; NEUTRINO; OSCILLATION; RADIATION; THEORETICAL MODEL;

EID: 42749102648     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.70.043006     Document Type: Article
Times cited : (40)

References (62)
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    • In particular, if we use the model of Eq. (8), the inclusion of MSW in the Earth diminishes the expected number of IBD events in KII (respectively in IMB) only by 0.5% (respectively by 2.5%). For the numerical evaluation, we use the formulas from F. Cavanna, M.L. Costantini, O. Palamara, and F. Vissani, astro-ph/0311256 in the approximation of uniform Earth density; for KII (respectively, IMB) the average density is (Formula presented) (respectively, 4.5) gr/cc, while the distance traveled in the Earth is (Formula presented) (respectively, 8500) km.
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    • Indeed, in certain astrophysical scenarios, as collapses with rotation 12, there is a large excess of (Formula presented) at production. What happens is similar to a (very) prolonged neutronization phase; the opacity of the medium is reduced, and energetic electron neutrinos free stream from the star, see also the reviews of V.S. Imshennik published in Astron. Lett. 18, 489 (1992)
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.