https://doi.org/10.1140/epjc/s10052-018-6038-z
Regular Article - Theoretical Physics
The origin of multi-TeV flares from the nearest blazar Markarian 421
1
Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Circuito Exterior, C.U., A. Postal 70-543, 04510, Mexico DF, Mexico
2
Astrophysical Big Bang Laboratory, RIKEN, Hirosawa, Wako, Saitama, 351-0198, Japan
3
Interdisciplinary Theoretical Science Research (iTHES), RIKEN, Hirosawa, Wako, Saitama, 351-0198, Japan
4
Interdisciplinary Theoretical and Mathematical Science (iTHEMS), RIKEN, Hirosawa, Wako, Saitama, 351-0198, Japan
5
Departamento de Física Aplicada, Centro de Investigacíon y de Estudios Avanzados del IPN Unidad Mérida, A. P. 73, Cordemex, 97310, Mérida, Yucatán, Mexico
* e-mail: sarira@nucleares.unam.mx
Received:
19
January
2018
Accepted:
25
June
2018
Published online:
7
July
2018
Markarian 421 is a high-peaked BL Lac object and it has undergone many strong outbursts since its discovery as a TeV source in 1992. Markarian 421 has been studied intensively and was observed by various Cherenkov telescope arrays ever since. The outbursts of April 2004 observed by the Whipple telescope and of February 2010 by the HESS telescopes are explained well in this work by using the photohadronic model. To account for the attenuation of these high-energy gamma-rays by the extragalactic background light (EBL), we use template EBL models. The intrinsic spectrum of each epoch is different even though the high-energy protons have almost the same spectral index. We observe that this difference in intrinsic spectra is due to the change in the spectral index of the low-energy tail of the synchrotron self Compton (SSC) photons during different epochs of flaring. Our results show that the contemporaneous multiwavelength observations, particularly in the low-energy tail region of the SSC emission of the source, are important in explaining the flaring phenomenon.
© The Author(s), 2018
