Unparticle constraints from supernova 1987A

Journal Article · Sat Dec 15 00:00:00 EST 2007 · Physical Review. D, Particles Fields

DOI:https://doi.org/10.1103/PHYSREVD.76.121701· OSTI ID:21023988

Hannestad, Steen ^[1]; Raffelt, Georg; Wong, Yvonne Y. Y. ^[2]

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1. Department of Physics and Astronomy, University of Aarhus, Ny Munkegade, DK-8000 Aarhus C (Denmark)
2. Max-Planck-Institut fuer Physik (Werner-Heisenberg-Institut), Foehringer Ring 6, D-80805 Munich (Germany)

The existence of an unparticle sector, weakly coupled to the standard model, would have a profound impact on supernova (SN) physics. Emission of energy into the unparticle sector from the core of SN 1987A would have significantly shortened the observed neutrino burst. The unparticle interaction with nucleons, neutrinos, electrons and muons is constrained to be so weak that it is unlikely to provide any missing-energy signature at colliders. One important exception are models where scale invariance in the hidden sector is broken by the Higgs vacuum expectation value. In this case the SN emission is suppressed by threshold effects.

• OSTI ID: 21023988
• Journal Information: Physical Review. D, Particles Fields, Vol. 76, Issue 12; Other Information: DOI: 10.1103/PhysRevD.76.121701; (c) 2007 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2821
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
ELECTRONS
EMISSION
EXPECTATION VALUE
HIGGS BOSONS
HIGGS MODEL
MUONS
NEUTRINOS
NUCLEONS
PARTICLE INTERACTIONS
SCALE INVARIANCE
STANDARD MODEL
SUPERNOVAE
VACUUM STATES