Dynamics of Temperature Distribution of Gravitationally Bound Objects in the Expanding Universe
https://doi.org/10.56304/S2079562920060445
Abstract
We consider a cluster of Primordial Black Holes (PBH) which is decoupled from the cosmological expansion (Hubble flow) and this region is heated as compared to the surrounding matter. The increased temperature inside the region can be explained by several mechanisms of PBH formation. The temperature dynamics is described by the appropriate equations in the framework of the Chapman–Enskog procedure.
About the Author
P. M. PetryakovaRussian Federation
Moscow, 115409
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Review
For citations:
Petryakova P.M. Dynamics of Temperature Distribution of Gravitationally Bound Objects in the Expanding Universe. Nuclear Physics and Engineering. 2021;12(2):129-131. (In Russ.) https://doi.org/10.56304/S2079562920060445