MGD Dirac Stars
Keyword(s):
The method of geometric deformation (MGD) is here employed to study compact stellar configurations, which are solutions of the effective Einstein–Dirac coupled field equations on fluid branes. Non-linear, self-interacting, fermionic fields are then employed to derive MGD Dirac stars, whose properties are analyzed and discussed. The MGD Dirac star maximal mass is shown to increase as a specific function of the spinor self-interaction coupling constant, in a realistic model involving the most strict phenomenological current bounds for the brane tension.
2006 ◽
Vol 306-308
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pp. 1223-1228
Keyword(s):
Keyword(s):
1993 ◽
Vol 182
(2-3)
◽
pp. 300-301
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2000 ◽
Vol 09
(05)
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pp. 543-549
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2019 ◽
Vol 28
(01)
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pp. 1950016
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2006 ◽
Vol 306-308
◽
pp. 1217-1222
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1976 ◽
Vol 55
(3)
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pp. 860-875
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