Fresh look at axions and SN 1987A

Wolfgang Keil, Hans-Thomas Janka, David N. Schramm, Günter Sigl, Michael S. Turner, and John Ellis
Phys. Rev. D 56, 2419 – Published 15 August 1997
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Abstract

We reexamine the very stringent limit on the axion mass based on the strength and duration of the neutrino signal from SN 1987A, in the light of new measurements of the axial-vector coupling strength of nucleons, possible suppression of axion emission due to many-body effects, and additional emission processes involving pions. The suppression of axion emission due to nucleon spin fluctuations induced by many-body effects degrades previous limits by a factor of about 2. Emission processes involving thermal pions can strengthen the limits by a factor of 3–4 within a perturbative treatment that neglects saturation of nucleon spin fluctuations. Inclusion of saturation effects, however, tends to make the limits less dependent on pion abundances. The resulting upper limit to the axion mass also depends on the precise couplings of the axion and ranges from 0.5×103 eV to 6×103 eV, consistent with previous results.

  • Received 23 December 1996

DOI:https://doi.org/10.1103/PhysRevD.56.2419

©1997 American Physical Society

Authors & Affiliations

Wolfgang Keil and Hans-Thomas Janka

  • Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, 85 740 Garching, Germany

David N. Schramm, Günter Sigl, and Michael S. Turner

  • Department of Astronomy and Astrophysics, Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637-1433
  • NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, Illinois 60510-0500

John Ellis

  • Theoretical Physics Division, CERN, CH-1211 Geneva 23, Switzerland

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Issue

Vol. 56, Iss. 4 — 15 August 1997

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