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1841
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1842
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1843
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1844“…The effect of multibody massless neutrino exchanges between neutrons inside a finite-size neutron star is studied. …”
Enlace del recurso
Enlace del recurso
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1845
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1846por Budagov, Yu A, Cundy, Donald C, Franzinetti, Carlo, Fretter, W B, Hopkins, H W K, Manfredotti, C, Myatt, Gerald, Nezrick, F A, Nikolic, Milan M, Novey, T B, Palmer, R B, Pattison, John Bryan M, Perkins, Donald Hill, Ramm, C A, Roe, B P, Stump, R, Venus, W A, Wachsmuth, H W, Yoshiki, HEnlace del recurso
Publicado 1969
Enlace del recurso
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1847por Budagov, Yu A, Cundy, Donald C, Franzinetti, Carlo, Fretter, W B, Hopkins, H W K, Manfredotti, C, Myatt, Gerald, Nezrick, F A, Nikolic, Milan M, Novey, T B, Palmer, R B, Pattison, John Bryan M, Perkins, Donald Hill, Ramm, C A, Roe, B P, Stump, R, Venus, W A, Wachsmuth, H W, Yoshiki, HEnlace del recurso
Publicado 1969
Enlace del recurso
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1848
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1849
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1850
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1851
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1852
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1853
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1854
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1855
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1856
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1857
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1858“…A neutrino of 1 MeV energy emits approximately $10^{-40}$ keV at $\tau=e\sqrt{2}G_F/\pi^2$. …”
Enlace del recurso
Enlace del recurso
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1859
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1860“…With one \Delta m^2 of the appropriate order of magnitude to solve the atmospheric neutrino problem, we study the resulting three-generation vacuum-oscillation fit to the solar neutrino flux. …”
Enlace del recurso
Enlace del recurso