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Phys. Rev. D 76, 121301(R) (2007) [4 pages]

Evidence for a new light spin-zero boson from cosmological gamma-ray propagation?

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Alessandro De Angelis*
Dipartimento di Fisica, Università di Udine, Via delle Scienze 208, I-33100 Udine and INAF and INFN, Sezioni di Trieste, Italy

Marco Roncadelli
Dipartimento di Fisica Nucleare e Teorica, Università di Pavia and INFN, Sezione di Pavia, Via A. Bassi 6, I-27100 Pavia, Italy

Oriana Mansutti
Dipartimento di Fisica, Università di Udine, Via delle Scienze 208, I-33100 Udine and INFN, Sezione di Trieste, Italy

Received 30 July 2007; revised 20 September 2007; published 18 December 2007

Recent findings by imaging atmospheric Cherenkov telescopes indicate a large transparency of the Universe to gamma rays, which can be hardly explained within the current models of extragalactic background light. We show that the observed transparency is naturally produced by an oscillation mechanism—which can occur inside intergalactic magnetic fields—whereby a photon can become a new spin-zero boson with mass m≪10-10  eV. Because the latter particle travels unimpeded throughout the Universe, photons can reach the observer even if the distance from the source considerably exceeds their mean free path. We compute the expected flux of gamma rays from blazar 3C279 at different energies. Our predictions can be tested in the near future by the gamma-ray telescopes H.E.S.S., MAGIC, CANGAROO, and VERITAS. Moreover, our result provides an important observational test for models of dark energy wherein quintessence is coupled to the photon through an effective dimension-five operator.

© 2007 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.76.121301
DOI:
10.1103/PhysRevD.76.121301
PACS:
95.85.Pw, 14.80.Mz

*Also at IST, Lisboa, Portugal.