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Axions from SN1987A
Abstract
Axion emission from SN1987A by nucleon-nucleon axion bremsstrahlung is considered. On the basis of the neutrino observations the axion luminosity must be \ensuremath{\lesssim}${10}^{53}$ erg ${\mathrm{s}}^{\mathrm{\ensuremath{-}}1}$. This occurs if (1) axions couple very weakly: ${m}_{a}$\ensuremath{\lesssim}0.75\ifmmode\times\else\texttimes\fi{}${10}^{\mathrm{\ensuremath{-}}3}$ eV; or (2) axions couple strongly enough to be ``trapped'' and radiated from an ``axion sphere'' with ${T}_{a}$\ensuremath{\lesssim}8 MeV: ${m}_{a}$\ensuremath{\gtrsim}2.2 eV. In general, ``axion trapping'' occurs for ${m}_{a}$\ensuremath{\gtrsim}0.016 eV. Our mass constraints are at best reliable to within a factor of \ensuremath{\simeq}3.
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Cites
Symmetry Breaking through Bell-Jackiw Anomalies
't Hooft, G. (1976) · Physical Review Letters · doi:10.1103/physrevlett.37.8 · Cited by 3,362
Cited by
Axions and the strongCPproblem
Kim, J. E., & Carosi, G. (2010) · Reviews of Modern Physics · doi:10.1103/revmodphys.82.557 · Cited by 916
Axions in inflationary cosmology
Linde, A. (1991) · Physics Letters B · doi:10.1016/0370-2693(91)90130-i · Cited by 773
The landscape of QCD axion models
Di Luzio, L., Giannotti, M., Nardi, E., & Visinelli, L. (2020) · Physics Reports · doi:10.1016/j.physrep.2020.06.002 · Cited by 657
Raffelt, G. G. (2008) · Lecture Notes in Physics · doi:10.1007/978-3-540-73518-2_3 · Cited by 566
Turner, M. S. (1990) · Physics Reports · doi:10.1016/0370-1573(90)90172-x · Cited by 489
Self-citation
Metadata
- Authors
- Turner, M. S.
- Venue
- Physical Review Letters
- Publisher
- American Physical Society (APS)
- Published
- 1988-05-02
- Volume
- 60
- Issue
- 18
- Pages
- 1797-1800
- ISSN
- 0031-9007 (ISSN-L)
- OpenAlex
- W1999001346
- Cited by
- 384
- References
- 1
- FWCI
- 21.11
- Type
- journal article
- Language
- en
- Open access
- closed
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