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Is cooling of a neutron star due to gravitational radiation?

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Publication:1054490
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DOI10.1007/BF01008388zbMath0519.70025OpenAlexW1965731671MaRDI QIDQ1054490

J. Blot

Publication date: 1983

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf01008388


zbMATH Keywords

cooling mechanism for neutron starsgravitational radiation emission by linear chaininterior of young starsthermal radiation of lattice structures


Mathematics Subject Classification ID

Lattice systems (Ising, dimer, Potts, etc.) and systems on graphs arising in equilibrium statistical mechanics (82B20) Gravitational waves (83C35) Classical field theories (70Sxx)


Related Items (2)

On gravitational radiation by a quantum bound system ⋮ Characteristic electromagnetic waves caused by tensorial and possible nontensorial thermal high-frequency gravitational waves from magnetars







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