Dimming Supernovae without Cosmic Acceleration

Csaba Csáki, Nemanja Kaloper, and John Terning
Phys. Rev. Lett. 88, 161302 – Published 9 April 2002
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Abstract

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 m1016eV, M4×1011GeV. This phenomenon may be an alternative to the accelerating Universe for explaining supernova observations.

  • Received 6 December 2001

DOI:https://doi.org/10.1103/PhysRevLett.88.161302

©2002 American Physical Society

Authors & Affiliations

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

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

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Vol. 88, Iss. 16 — 22 April 2002

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