Time evolution of rotating and magnetized white dwarf stars

Author:

Becerra L12,Boshkayev K34ORCID,Rueda J A125,Ruffini R125

Affiliation:

1. ICRANet, Piazza della Repubblica 10, I–65122 Pescara, Italy

2. Dipartimento di Fisica and ICRA, Sapienza Università di Roma, P.le Aldo Moro 5, I–00185 Rome, Italy

3. NNLOT, al-Farabi Kazakh National University, Al-Farabi av. 71, 050040 Almaty, Kazakhstan

4. Department of Physics, Nazarbayev University, Kabanbay Batyr 53, 010000 Astana, Kazakhstan

5. ICRANet-Rio, CBPF, Rua Dr. Xavier Sigaud 150, Rio de Janeiro, RJ, 22290–180, Brazil

Funder

Ministry of Education and Science

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 7 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. On the Optical Transients from Double White-dwarf Mergers;The Astrophysical Journal;2023-11-20

2. The Double White Dwarf Merger Progenitors of SDSS J2211+1136 and ZTF J1901+1458;The Astrophysical Journal;2022-12-01

3. Massive white dwarfs in $$f(\mathtt {R,L_m})$$ gravity;The European Physical Journal C;2022-06-18

4. The white dwarf binary merger model of GRB 170817A;International Journal of Modern Physics D;2022-02-16

5. Near-Chandrasekhar-mass Type Ia Supernovae from the Double-degenerate Channel;The Astrophysical Journal;2022-01-01

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