A cosmological upper limit on the mass of heavy neutrinos

P. Hut, K. A. Olive

Research output: Contribution to journalArticlepeer-review

36 Scopus citations

Abstract

An upper limit of 60 GeV is derived on the mass of a stable heavy neutrino, using the standard big bang model. This is in addition to the previous limits which constrain the mass of a neutrino to be less than 50 eV or greater than 10 GeV. Thus, we predict that in the near future all existing types of stable neutrinos will be detected.

Original languageEnglish (US)
Pages (from-to)144-146
Number of pages3
JournalPhysics Letters B
Volume87
Issue number1-2
DOIs
StatePublished - Oct 22 1979
Externally publishedYes

Bibliographical note

Funding Information:
This work has been stimulated by the Summer School on Physical Cosmology at Les Houches We would hke to thank J Audouze and R Kochhar for their assistance in preparing this paper We would also hke to thank D N Schramm, P J E Peebles and G A Tammann for valuable discussions This work has been supported in part by the Fanme and John Hertz Foundation and NSF grant AST 78-21402 at the University of Ctucago

Fingerprint Dive into the research topics of 'A cosmological upper limit on the mass of heavy neutrinos'. Together they form a unique fingerprint.

Cite this