CMB bispectrum from primordial magnetic fields on large angular scales

K. Jedamzik, V. Katalinic, and A. Olinto, Phys. Rev. D57

1998

Earlier work this paper cites.

T. R. Seshadri and K. Subramanian, Phys. Rev. Lett., 87

2002

Earlier work this paper cites.

C. Caprini, R. Durrer, Phys. Rev. D, 65

2002

Earlier work this paper cites.

K. Subramanian, T. R. Seshadri and J. D. Barrow, Mon. Not. Roy. Astr. Soc., 344

2003

Earlier work this paper cites.

H. K. Moffatt, Magnetic Field Generation in Electrically Conducting Fluids, Cambridge University Press, Cambridge (1978); F. Krause, K.-H. Rädler, Mean-field magnetohydrodynamics and dynamo theory, Pergamon Press, Oxford (1980); A. A. Ruzmaikin, A. Shukurov and D. Sokoloff, Magnetic Fields of Galaxies

2005

Earlier work this paper cites.

I. Brown, and R. Crittenden, Phys. Rev. D, 72

2005

Earlier work this paper cites.

M. Turner, L. M. Widrow, Phys. Rev. D. 37

2007

Cited alongside, same era.

M. Giovannini, PMC Physics A, 1

2007

Cited alongside, same era.

J. R. Fergusson and E. P. S. Shellard, Phys. Rev. D, 76

2007

Cited alongside, same era.

K. Subramanian, Astron. Nach., 327

2007

Cited alongside, same era.

J. D. Barrow, P. G. Ferreira and J. Silk, Phys. Rev. Lett., 78

2008

Cited alongside, same era.

The WMAP 5-year data gives limits on primordial non-Gaussianity − 9 < f N ​ L l ​ o ​ c ​ a ​ l < 111 -9<f_{NL}^{local}<111 and − 151 < f N ​ L e ​ q ​ u ​ i ​ l < 253 -151<f_{NL}^{equil}<253 at the 95 % 95\% confidence level for the local and equilateral models, respectively. Of course these limits use the much larger range of l l values than the range for which the SW contribution is important

G. Chen, P. Mukherjee, T. Kahniashvili, B. Ratra and Yun Wang, Astrophys.J., 611

2008

Later among the works it cites.

D. Paoletti, F. Finelli and F. Paci, arxiv:0811.0230 (2008)

Original

2008

Later among the works it cites.

A. Riotto, The quest for Non-Gaussianity

2008

Later among the works it cites.

E. Komatsu et al., Astrophys. J. Suppl. 180

2009

Closest in time.

C. Caprini, F. Finelli, D. Paoletti and A. Riotto, arxiv:0903.1420 (2009)

Original

2009

Closest in time.