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Comment on "Zero temperature, degenerate fermion stars" [S. Boatto, M.B. Paranjape, V. Pessanha, C.A.D. Zarro. ArXiv: 2609.20950]

Abstract

In contrast to S. Boatto et al. \cite{Boat}, the degree of compactification or compactness is clarified for the self-gravitating spheric star of fermionic matter.

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BibTeX
@misc{burmistrov2026comment,
  title = {{Comment on "Zero temperature, degenerate fermion stars" [S. Boatto, M.B. Paranjape, V. Pessanha, C.A.D. Zarro. ArXiv: 2609.20950]}},
  author = {Serguei N. Burmistrov},
  howpublished = {arXiv},
  year = {2026},
  month = nov,
  doi = {10.48550/arxiv.2611.01103},
  eprint = {2611.01103},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2611.01103},
}
RIS
TY  - UNPB
TI  - Comment on "Zero temperature, degenerate fermion stars" [S. Boatto, M.B. Paranjape, V. Pessanha, C.A.D. Zarro. ArXiv: 2609.20950]
AU  - Serguei N. Burmistrov
PY  - 2026
DA  - 2026/11/01
PB  - arXiv
DO  - 10.48550/arxiv.2611.01103
UR  - https://arxiv.org/abs/2611.01103
AB  - In contrast to S. Boatto et al. \cite{Boat}, the degree of compactification or compactness is clarified for the self-gravitating spheric star of fermionic matter.
ER  -