Solution of the Inverse Problem of the Transfer of Ultrarelativistic Nuclei in the Expanding Universe


Дәйексөз келтіру

Толық мәтін

Ашық рұқсат Ашық рұқсат
Рұқсат жабық Рұқсат берілді
Рұқсат жабық Тек жазылушылар үшін

Аннотация

We consider propagation of nuclei with energies over 1018 eV in the expanding Universe filled with background electromagnetic radiation. The spectrum of sources of extragalactic cosmic rays for protons and nuclei up to iron is determined on the basis of the particle spectrum observed near Earth as a solution of the inverse problem of transfer of ultrarelativistic nuclei. The method of regularization of the solution of this mathematically ill-posed problem is used basing on the data of the Pierre Auger Observatory on the energy spectrum of cosmic rays, the average logarithm of the mass number, and its variance. The found energy spectra of the sources prove to be very hard and strongly dependent on the assumption about the composition of the accelerated nuclei.

Авторлар туралы

V. Zirakashvili

N. V. Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of the Russian Academy of Sciences (IZMIRAN)

Email: vptuskin@azmiran.ru
Ресей, Moscow

V. Ptuskin

N. V. Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of the Russian Academy of Sciences (IZMIRAN)

Хат алмасуға жауапты Автор.
Email: vptuskin@azmiran.ru
Ресей, Moscow

S. Rogovaya

N. V. Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of the Russian Academy of Sciences (IZMIRAN)

Email: vptuskin@azmiran.ru
Ресей, Moscow

Қосымша файлдар

Қосымша файлдар
Әрекет
1. JATS XML

© Springer Science+Business Media New York, 2017