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Dense Nuclear Matter in a Strong Magnetic Field
Open accessAbstract
We investigate in a relativistic Hartree theory the gross properties of cold symmetric nuclear matter and nuclear matter in beta equilibrium under the influence of strong magnetic fields. If the field strengths are above the critical values for electrons and protons, the respective phase spaces are strongly modified. This results in additional binding of the systems with distinctively softer equations of state compared to the field free cases. For magnetic field $\ensuremath{\sim}{10}^{20}$ G and beyond, the nuclear matter in beta equilibrium practically converts into a stable proton-rich matter.
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Citations
Cited by
Matter in strong magnetic fields
Lai, D. (2001) · Reviews of Modern Physics · doi:10.1103/revmodphys.73.629 · Cited by 540
The Equation of State of Neutron Star Matter in Strong Magnetic Fields
Broderick, A., Prakash, M., & Lattimer, J. M. (2000) · The Astrophysical Journal · doi:10.1086/309010 · Cited by 338
Equation of state of a dense and magnetized fermion system
Ferrer, E. J., de la Incera, V., Keith, J. P., Portillo, I., & Springsteen, P. L. (2010) · Physical Review C · doi:10.1103/physrevc.82.065802 · Cited by 314
Metadata
- Authors
- Chakrabarty, S., Bandyopadhyay, D., & Pal, S.
- Venue
- Physical Review Letters
- Publisher
- American Physical Society (APS)
- Published
- 1997-04-14
- Volume
- 78
- Issue
- 15
- Pages
- 2898-2901
- ISSN
- 0031-9007 (ISSN-L)
- 1079-7114
- OpenAlex
- W1994046488
- Cited by
- 207
- References
- 0
- FWCI
- 4.44
- Type
- journal article
- Language
- en
- Open access
- green
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- Chakrabarty, S., Bandyopadhyay, D., & Pal, S. (1997). Dense Nuclear Matter in a Strong Magnetic Field. Physical Review Letters. https://doi.org/10.1103/physrevlett.78.2898
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