HEATING OF A MOLECULAR CLOUD BY A PRIMORDIAL BLACK HOLE
- Авторлар: Melikhov A.N.1, Mikheeva E.V.1
-
Мекемелер:
- Astro Space Center of the P. N. Lebedev Physical Institute Russian Academy of Sciences
- Шығарылым: Том 166, № 5 (2024)
- Беттер: 618-631
- Бөлім: NUCLEI, PARTICLES, FIELDS, GRAVITY AND ASTROPHYSICS
- URL: https://journals.rcsi.science/0044-4510/article/view/268671
- DOI: https://doi.org/10.31857/S0044451024110051
- ID: 268671
Дәйексөз келтіру
Аннотация
The heating of a molecular cloud by photons emitted by a primary black hole (PBH) located inside the cloud is considered. For graphite and silicate dust particles, the dependence of dust temperature on the distance from PBH is derived, along with the emission spectrum of dust particles. The obtained spectrum is compared with the sensitivity of the Millimetron space observatory for various values of concentration and size of dust particles and different PBH masses.
Авторлар туралы
A. Melikhov
Astro Space Center of the P. N. Lebedev Physical Institute Russian Academy of Sciences
Email: melikhov94@inbox.ru
Ресей, 117997, Moscow
E. Mikheeva
Astro Space Center of the P. N. Lebedev Physical Institute Russian Academy of Sciences
Хат алмасуға жауапты Автор.
Email: helen@asc.rssi.ru
Ресей, 117997, Moscow
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