Gamma-ray observations of blazars and the intergalactic magnetic field spectrum

被引:49
作者
Caprini, C. [1 ,2 ]
Gabici, S. [3 ]
机构
[1] CNRS, URA 2306, F-91191 Gif Sur Yvette, France
[2] CEA, IPhT, F-91191 Gif Sur Yvette, France
[3] Univ Paris Diderot, Obs Paris, CEA Irfu, Sorbonne Paris Cite,APC,CNRS,IN2P3, F-75013 Paris, France
来源
PHYSICAL REVIEW D | 2015年 / 91卷 / 12期
关键词
TEV LIGHT CURVES; LOWER BOUNDS; EMISSION; RADIATION; PHOTONS; CASCADE; SEARCH; FLARE;
D O I
10.1103/PhysRevD.91.123514
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Very high-energy observations of blazars can be used to constrain the strength of the intergalactic magnetic field. A simplifying assumption which is often made is that of a magnetic field of constant strength composed of randomly oriented and identical cells. In this paper, we demonstrate that a more realistic description of the structure of the intergalactic magnetic field is indeed needed. If such a description is adopted, the observational bounds on the field strength are significantly affected in the limit of short field correlation lengths: in particular, they acquire a dependence on the magnetic field power spectrum. In the case of intergalactic magnetic fields which are generated causally, for which the magnetic field large-scale spectral index is n(B) >= 2 and even, the observational lower bound becomes more constraining by about a factor of 3. If instead -3 < n(B) < -2, the lower bound is significantly relaxed. Such magnetic fields with very red spectra can in principle be produced during inflation, but remain up to now speculative.
引用
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页数:10
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