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Interstellar neutrino density and cosmogony

  • Published:
Acta Physica Academiae Scientiarum Hungaricae

Abstract

The cosmic neutrino density hitherto produced by the stars is estimated. Experimental determination of this quantity would be of great importance and any discrepancy between estimated and experimental value would be of great consequence for cosmogony. A brief review of the indirect (gravitational) and direct (atomphysical) possibilities of observation is given.

Резюме

Оценивается плотность космических нейтрино как продуктов термоядерных реакций звёзд и супернов. Наблюдение большей нлотности нейтрино указывало бы на сигнулярное (дозвездное) состояние материи. Нодробно истолкуются гравитационное влияние нейтринного фона и непосредственные возможности наблюдения мягкой компоненты нейтринного излучения двух видов.

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Author notes

  1. L. Fodor

    Present address: Observatory of the Hungarian Academy of Sciences, Budapest-Szabadsághegy

  2. Zs. Kövesy

    Present address: Central Research Institute of Physics, Budapest

Authors and Affiliations

  1. Institute for Theoretical Physics, Roland Eötvös University, Budapest

    L. Fodor, Zs. Kövesy & G. Marx

Authors
  1. L. Fodor
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  2. Zs. Kövesy
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  3. G. Marx
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Fodor, L., Kövesy, Z. & Marx, G. Interstellar neutrino density and cosmogony. Acta Phys. Hung. 17, 171–183 (1964). https://doi.org/10.1007/BF03156901

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  • DOI: https://doi.org/10.1007/BF03156901

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