Spacetime Exterior to a Star: Against Asymptotic Flatness
In many circumstances the perfect fluid conservation equations can be directly integrated to give a geometric-thermodynamic equation: typically that the lapse N is the reciprocal of the enthalphy h, (N = 1/h). This result is aesthetically appealing as it depends only on the fluid conservation equati...
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| Format: | Article |
| Language: | English |
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De Gruyter
2016-01-01
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| Series: | Open Physics |
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| Online Access: | https://doi.org/10.1515/phys-2016-0043 |