| Texto completo | |
| Autor(es): |
Número total de Autores: 2
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| Afiliação do(s) autor(es): | [1] Univ Fed ABC, Ctr Ciencias Nat & Humanas, Ave Estados 5001 Bangu, BR-09210580 Santo Andre, SP - Brazil
[2] Comis Nacl Energia Atom, Dept Fis, Av Libertador 8250, RA-1429 Buenos Aires, DF - Argentina
[3] Consejo Nacl Invest Cient & Tecn, RA-2290 Buenos Aires, DF - Argentina
Número total de Afiliações: 3
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| Tipo de documento: | Artigo Científico |
| Fonte: | UNIVERSE; v. 7, n. 12 DEC 2021. |
| Citações Web of Science: | 0 |
| Resumo | |
We review the properties of hybrid stars with a quark matter core and a hadronic mantle, focusing on the role of key micro-physical properties such as the quark/hadron surface and curvature tensions and the conversion speed at the interface between both phases. We summarize the results of works that have determined the surface and curvature tensions from microscopic calculations. If these quantities are large enough, mixed phases are energetically suppressed and the quark core would be separated from the hadronic mantle by a sharp interface. If the conversion speed at the interface is slow, a new class of dynamically stable hybrid objects is possible. Densities tens of times larger than the nuclear saturation density can be attained at the center of these objects. We discuss possible formation mechanisms for the new class of hybrid stars and smoking guns for their observational identification. (AU) | |
| Processo FAPESP: | 13/10559-5 - Investigação de fenômenos de altas energias e plasmas astrofísicos: teoria, simulações numéricas, observações e desenvolvimento de instrumentação para o Cherenkov Telescope Array (CTA) |
| Beneficiário: | Elisabete Maria de Gouveia Dal Pino |
| Modalidade de apoio: | Auxílio à Pesquisa - Projetos Especiais |