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pro vyhledávání: '"Mourelle, Jorge Castelo"'
Rotating bosonic dark matter halos are considered as potential candidates for modeling dark matter in galactic halos. These bosonic dark matter halos can be viewed as a dilute and very extended version of bosonic stars, and the methods used for the c
Externí odkaz:
http://arxiv.org/abs/2407.07839
Autor:
Adam, Christoph, Mourelle, Jorge Castelo, Filho, Etevaldo dos Santos Costa, Herdeiro, Carlos A. R., Wereszczynski, Andrzej
Bosonic stars represent a hypothetical exotic type of compact stellar objects that could be observed from the gravitational signal of coalescing binaries in current and future gravitational wave detectors. There are two main families of bosonic stars
Externí odkaz:
http://arxiv.org/abs/2406.07613
Rotating fermion-boson stars are hypothetical celestial objects that consist of both fermionic and bosonic matter interacting exclusively through gravity. Bosonic fields are believed to arise in certain models of particle physics describing dark matt
Externí odkaz:
http://arxiv.org/abs/2403.13052