V. I. Romansky, A. M. Bykov, S. M. Osipov, A. A. Lutovinov
{"title":"Can Fast Blue Optical Transients be Cosmic Pevatrons?","authors":"V. I. Romansky, A. M. Bykov, S. M. Osipov, A. A. Lutovinov","doi":"10.1134/S1062873825711547","DOIUrl":null,"url":null,"abstract":"<p>The new class of recently discovered astrophysical objects—fast blue optical transients (FBOT) demonstrated a high luminosity of radio and X-ray radiation and the expansion velocities above 0.1 c over a year time scale. They are likely sub-class of core-collapse supernova events. We present here results of modeling of particle acceleration in mildly-relativistic shocks associated with FBOTs. It is shown, that objects with mildly-relativistic shocks can be possible sources of particles with energies above 1 PeV, and emit detectable fluxes of hard X-ray radiation.</p>","PeriodicalId":504,"journal":{"name":"Bulletin of the Russian Academy of Sciences: Physics","volume":"89 6","pages":"993 - 997"},"PeriodicalIF":0.4800,"publicationDate":"2025-07-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Bulletin of the Russian Academy of Sciences: Physics","FirstCategoryId":"1085","ListUrlMain":"https://link.springer.com/article/10.1134/S1062873825711547","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"Physics and Astronomy","Score":null,"Total":0}
引用次数: 0
Abstract
The new class of recently discovered astrophysical objects—fast blue optical transients (FBOT) demonstrated a high luminosity of radio and X-ray radiation and the expansion velocities above 0.1 c over a year time scale. They are likely sub-class of core-collapse supernova events. We present here results of modeling of particle acceleration in mildly-relativistic shocks associated with FBOTs. It is shown, that objects with mildly-relativistic shocks can be possible sources of particles with energies above 1 PeV, and emit detectable fluxes of hard X-ray radiation.
期刊介绍:
Bulletin of the Russian Academy of Sciences: Physics is an international peer reviewed journal published with the participation of the Russian Academy of Sciences. It presents full-text articles (regular, letters to the editor, reviews) with the most recent results in miscellaneous fields of physics and astronomy: nuclear physics, cosmic rays, condensed matter physics, plasma physics, optics and photonics, nanotechnologies, solar and astrophysics, physical applications in material sciences, life sciences, etc. Bulletin of the Russian Academy of Sciences: Physics focuses on the most relevant multidisciplinary topics in natural sciences, both fundamental and applied. Manuscripts can be submitted in Russian and English languages and are subject to peer review. Accepted articles are usually combined in thematic issues on certain topics according to the journal editorial policy. Authors featured in the journal represent renowned scientific laboratories and institutes from different countries, including large international collaborations. There are globally recognized researchers among the authors: Nobel laureates and recipients of other awards, and members of national academies of sciences and international scientific societies.