Constraints on supernovae dimming from photon-pseudo scalar coupling

نویسندگان

  • Yong-Seon Song
  • Wayne Hu
چکیده

An alternative mechanism that dims high redshift supernovae without cosmic acceleration utilizes an oscillation of photons into a pseudo-scalar particle during transit. Since angular diameter distance measures are immune to the loss of photons, this ambiguity in interpretation can be resolved by combining CMB acoustic peak measurements with the recent baryon oscillation detection in galaxy power spectra. This combination excludes a non-accelerating dark energy species at the 4σ level regardless of the level of the pseudo-scalar coupling. While solutions still exist with substantial non-cosmological dimming of supernovae, they may be tested with future improvement in baryon oscillation experiments.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Photon-axion conversion as a mechanism for supernova dimming: Limits from CMB spectral distortion

Axion-photon conversion induced by intergalactic magnetic fields has been proposed as an explanation for the dimming of distant supernovae of type Ia (SNe Ia) without cosmic acceleration. The effect depends on the intergalactic electron density ne as well as the B-field strength and domain size. We show that for ne < ∼ 10 cm the same mechanism would cause excessive spectral distortion of the co...

متن کامل

Exorcising W < −1

We show that the combined dimming of Type Ia supernovae induced by both a cosmological constant and the conversion of photons into axions in extra-galactic magnetic fields can impersonate dark energy with an equation of state w < −1. An observer unaware of the presence of photon-axion conversion would interpret the additional dimming as cosmic acceleration faster than that induced by a cosmolog...

متن کامل

Sgoldstinos: Primaries of Ultra-high Energy Cosmic Rays

In any model with supersymetry being spontaneously broken exists goldstino supermultiplet. In a set of models (pseudo)scalar superpartners of goldstino (sgoldstinos) are light (m < 1 GeV), long-living and sufficiently strongly interacting. There are some puzzles in astrophysics and cosmology without relevant solutions in the framework of the Standard Model. In particular, Ultra High Energy Cosm...

متن کامل

Cosmic Acceleration Vs Axion-photon Mixing

Axion-photon mixing has been proposed as an alternative to acceleration as the explanation for supernovae dimming. We point out that the loss of photons due to this mixing will induce a strong asymmetry between the luminosity, dL(z), and angular-diameter distance, dA(z), since the latter is unaffected by mixing. In a first search for such asymmetry we introduce an amplitude A, such that A = 1 i...

متن کامل

Super-GZK Photons from Photon-Axion Mixing

We show that photons with energies above the GZK cutoff can reach us from very distant sources if they mix with light axions in extragalactic magnetic fields. The effect which enables this is the conversion of photons into axions, which are sufficiently weakly coupled to travel large distances unimpeded. These axions then convert back into high energy photons close to the Earth. We show that ph...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2005