ON THE POST-LINEAR QUADRUPOLE-QUADRUPOLE METRIC
The Hartle-Thorne metric defines a reliable spacetime for most as- trophysical purposes, for instance simulations of slowly rotating stars. Solving the Einstein field equations, we added terms of second order in the quadrupole moment to its post-linear version in order to compare it with solutions f...
I tiakina i:
| I whakaputaina i: | Revista de Matemática: Teoría y Aplicaciones |
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| Ngā kaituhi matua: | , |
| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
Universidad de Costa Rica
2017
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| Ngā marau: | |
| Urunga tuihono: | https://www.redalyc.org/articulo.oa?id=45352200003 |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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