1998ApJ...509..537P -
Astrophys. J., 509, 537-543 (1998/December-3)
Gamma-ray bursts from baryon decay in neutron stars.
PEN U.-L., LOEB A. and TUROK N.
Abstract (from CDS):
The standard unbroken electroweak theory is known to erase the baryon number. The baryon number symmetry can be restored in the core of a neutron star if its density diverges via gravitational instability due to a binary merger event. We argue that for certain double Higgs models with discrete symmetries this process may result in an expanding self-sustained burning front that would convert the entire neutron matter into radiation. This process would release ∼1054 ergs in electromagnetic radiation over ∼10–4 s with negligible baryonic contamination. The resulting fireball would have all of the properties necessary to produce a γ-ray burst as a result of its interaction with ambient interstellar gas. The subsequent Higgs decay would produce a millisecond burst of ∼1052 ergs in ∼100 GeV neutrinos, which might be observable. The above mechanism may also cause electroweak baryogenesis in the early universe, which gives rise to the observed matter-antimatter asymmetry today.
Abstract Copyright:
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Journal keyword(s):
Cosmology: Theory - Gamma Rays: Bursts - Stars: Neutron
Simbad objects:
2
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