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Updated: Jun 5, 2025

Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
Supernova Axions Convert to Gamma Rays in Magnetic Fields of Progenitor Stars
Claudio Andrea Manzari1, Yujin Park1, Benjamin R Safdi1
1Berkeley Center for Theoretical Physics, <a href="https://ror.org/01an7q238">University of California</a>, Berkeley, California 94720, USA and Theoretical Physics Group, <a href="https://ror.org/02jbv0t02">Lawrence Berkeley National Laboratory</a>, Berkeley, California 94720, USA.
Supernova observations constrain axion properties. Future gamma-ray telescopes could detect axions (hypothetical particles) from supernovae and neutron star mergers, aiding dark matter research.
Area of Science:
- Astrophysics
- Particle Physics
- Cosmology
Background:
- Axions are hypothetical particles that could be produced in supernovae.
- Previous studies constrained low-mass axions (m_a ≲ 10^-10 eV) using SN1987A gamma-ray non-observations.
- Higher-mass axions remain largely unconstrained.
Purpose of the Study:
- To constrain higher-mass axions (up to m_a ~ 10^-3 eV) using SN1987A data.
- To explore the potential of future galactic supernovae for detecting axions.
- To propose a new instrument for detecting axion signals.
Main Methods:
- Analyzing axion production mechanisms: Primakoff process, nucleon bremsstrahlung, and pion conversion.
- Modeling axion-to-gamma-ray conversion in progenitor star magnetic fields.
- Utilizing SN1987A observations and proposing future observational strategies.
Main Results:
- SN1987A data provides constraints on axions with masses up to ~10^-3 eV.
- Future galactic supernovae could detect quantum chromodynamics (QCD) axions with masses > 50 μeV.
- The proposed GALactic AXion Instrument for Supernova (GALAXIS) could detect axion signals from future events.
Conclusions:
- SN1987A is a valuable tool for constraining axion properties across a wider mass range.
- Future supernova observations offer a promising avenue for discovering axions.
- The GALAXIS mission could significantly advance the search for axions and related phenomena.
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