Particle Physics from Stars
arXiv:hep-ph/9903472 · doi:10.1146/annurev.nucl.49.1.163
Abstract
Low-mass particles such as neutrinos, axions, other Nambu-Goldstone bosons and gravitons are produced in the hot and dense interior of stars. Therefore, astrophysical arguments constrain the properties of these particles in ways which are often complementary to cosmological arguments and to laboratory experiments. This review provides an update on the most important stellar-evolution limits and discusses them in the context of other information from cosmology and laboratory experiments.
46 pages, including 14 eps figures, prepared for vol.49 of the Annual Review of Nuclear and Particle Science (1999)
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Cited by in corpus (230)
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- Helioscope Bounds on Hidden Sector Photons
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- New Light Species and the CMB
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- Dark Matter Candidates - Axions, Neutralinos, Gravitinos, and Axinos
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- Reverse Direct Detection: Cosmic Ray Scattering With Light Dark Matter
- Supernova Neutrino Burst Detection with the Deep Underground Neutrino Experiment
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- The Cosmology of Sub-MeV Dark Matter
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- Anomaly induced effects in a magnetic field
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- Signatures of Pseudoscalar Photon Mixing in CMB Radiation
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- Solar flux: Revisiting bounds on neutrino magnetic moments and solar magnetic field
- Constraining axionlike particles using the distance-duality relation
- Constraints on non-resonant photon-axion conversion from the Planck satellite data
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- A model for right-handed neutrino magnetic moments
- Polarization-operator approach to optical signatures of axion-like particles in strong laser pulses
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- Leptogenesis from oscillations and dark matter
- Probing Heavy Sterile Neutrinos at Ultrahigh Energy Neutrino Telescopes via the Dipole Portal
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- New limit on pseudoscalar-photon mixing from WMAP Observations
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- Stars and Fundamental Physics
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- Axion Electrodynamics in Strong Magnetic Backgrounds