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Phys. Rev. Lett. 88, 161302 (2002) [4 pages]

Dimming Supernovae without Cosmic Acceleration

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Csaba Csáki1,*, Nemanja Kaloper2, and John Terning1
1Theory Division T-8, Los Alamos National Laboratory, Los Alamos, New Mexico 87545
2Department of Physics, Stanford University, Stanford, California 94305

Received 6 December 2001; published 9 April 2002

We present a simple model where photons propagating in extragalactic magnetic fields can oscillate into very light axions. The oscillations may convert some of the photons, departing a distant supernova, into axions, making the supernova appear dimmer and hence more distant than it really is. Averaging over different configurations of the magnetic field we find that the dimming saturates at about one-third of the light from the supernovae at very large redshifts. This results in a luminosity distance versus redshift curve almost indistinguishable from that produced by the accelerating Universe, if the axion mass and coupling scale are m10-16eV, M4×1011GeV. This phenomenon may be an alternative to the accelerating Universe for explaining supernova observations.

© 2002 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.88.161302
DOI:
10.1103/PhysRevLett.88.161302
PACS:
98.80.Cq, 14.80.Mz, 97.60.Bw

*Current address: Newman Laboratory of Nuclear Studies, Cornell University, Ithaca, New York 14853.