Limits for primordial magnetic fields

K. Subramanian and J.D. Barrow, Phys. Rev. D58, 083502 (1998)

1998

Earlier work this paper cites.

R. Durrer and C. Caprini, JCAP 0311, 010 (2003)

2003

Earlier work this paper cites.

D. Grasso and H. Rubinstein, Phys. Rept. 348, 163 (2001); M. Giovannini, Int. J. Mod. Phys. D 13, 391 (2004)

2004

Earlier work this paper cites.

R. Banerjee and K. Jedamzik, Phys. Rev. D70, 123003 (2004)

2004

Earlier work this paper cites.

C. Caprini et al, Phys.Rev. D69, 063006 (2004)

2004

Earlier work this paper cites.

K. Subramanian et al, MNRAS 344, L31 (2003); A. Lewis, Phys. Rev. D70, 043011 (2004)

2004

Earlier work this paper cites.

A. Brandenburg and K. Subramanian, Phys. Rept. 417, 1 (2005)

2005

Cited alongside, same era.

C. Caprini and R. Durrer, Phys.Rev. D65, 023517 (2001); C. Caprini and R. Durrer, Phys. Rev. D72, 088301 (2005)

2005

Cited alongside, same era.

See for example R. Beck, ASTRA 5, 43 (2009); P.P. Kronberg et al, Astrophys. J. 676, 7079 (2008); M.L. Bernet et al, Nature 454, 302 (2008); L. Pentericci et al, A&A Supp. Ser. 145, 121 (2000); M. Thierbach et al, A&A 397, 53 (2003); F. Govoni and L. Feretti, Int. J. Mod. Phys. D13, 1549 (2004); C. Vogt and T.A. Ensslin, A&A 434, 67 (2005); D. Guidetti et al, A&A 483, 699 (2008); A. Bonafede et al, A&A 513, A30 (2010); Y. Xu et al, Astrophys. J. 637, 19 (2006)

2006

Cited alongside, same era.

P.A. Davidson, Turbulence (Oxford University Press, Oxford, 2004); D.T. Son, Phys. Rev. D 59, 63008 (1999); M.R. Smith et al, Phys. Rev. Lett. 71, 2583 (1993); D. Biskamp and W.C. Muller, Phys. Rev. Lett. 83, 2195 (1999); M. Christensson et al, Phys. Rev. E 64, 056405 (2001); L. Campanelli, Phys. Rev. D 70, 083009 (2004); L. Campanelli, Phys. Rev. Lett. 98, 251302 (2007)

C. Caprini et al, JCAP 0906, 021 (2009)

2009

Later among the works it cites.

T. Kahniashvili et al, Phys. Rev. D81, 123002 (2010); K. Jedamzik and G. Sigl, arXiv:1012.4794

Original

2010

Later among the works it cites.

M. Giovannini and K. Kunze, Phys. Rev. D77, 123001 (2008); D.G. Yamazaki et al, Phys. Rev. D77 043005 (2008); F. Finelli et al, Phys. Rev. D78, 023510 (2008); D. Paoletti et al, MNRAS 396, 523 (2009); R. Shaw and A. Lewis, Phys. Rev D82, 121302 (2010); D.G. Yamazaki et al, Phys. Rev. D81, 023008 (2010); K. Kunze, arXiv:1007.3163 [astro-ph.CO]

Original

2010

Later among the works it cites.

I. Brown and R. Crittenden, Phys. Rev. D72, 063002 (2005); T.R. Seshadri and K. Subramanian, Phys. Rev. Lett. 103, 081303 (2009); P. Trivedi et al, arXiv:1009.2724 [astro-ph.CO]; M. Shiraishi et al, Phys. Rev. D82, 121302 (2010)

Original

2010

Later among the works it cites.