Diskussion:Tolman-Oppenheimer-Volkoff-Grenze
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Artikel ist eine Überstzung des englischen Wikipedia Artikels en:Tolman-Oppenheimer-Volkoff Limit. Die ursprünglichen Autoren sind folgende:
* (cur) (last) 00:15, 3 April 2007 Christopher Thomas (Talk | contribs) (rv. External sources use "Volkoff" as the spelling.) * (cur) (last) 00:05, 3 April 2007 129.82.217.154 (Talk) * (cur) (last) 00:04, 3 April 2007 129.82.217.154 (Talk) * (cur) (last) 00:02, 3 April 2007 129.82.217.154 (Talk) * (cur) (last) 03:19, 31 January 2007 Melamed katz (Talk | contribs) m (interwiki) * (cur) (last) 00:24, 28 January 2007 Spacepotato (Talk | contribs) (Revise value, slight rewrite, +cat, +see also) * (cur) (last) 14:51, 25 January 2007 Bota47 (Talk | contribs) m (robot Modifying: cs:Tolmanova-Oppenheimerova-Volkoffova mez) * (cur) (last) 22:07, 12 January 2007 Urhixidur (Talk | contribs) (Who they wer) * (cur) (last) 19:22, 11 January 2007 Gveret Tered (Talk | contribs) m (interwiki) * (cur) (last) 18:52, 9 December 2006 RJHall (Talk | contribs) (ref.) * (cur) (last) 18:46, 9 December 2006 RJHall (Talk | contribs) (needs refs; paragraph breaks) * (cur) (last) 21:06, 28 November 2006 Incnis Mrsi (Talk | contribs) m (ru:Предел Оппенгеймера — Волкова) * (cur) (last) 14:48, 18 November 2006 Lynxara (Talk | contribs) * (cur) (last) 21:56, 10 November 2006 WolfmanSF (Talk | contribs) (Delete "experimental", since such evidence might be observational.) * (cur) (last) 20:08, 4 November 2006 WolfmanSF (Talk | contribs) (Add link to "quark degeneracy".) * (cur) (last) 20:03, 4 November 2006 WolfmanSF (Talk | contribs) m (Add link to "degenerate matter".) * (cur) (last) 19:59, 4 November 2006 WolfmanSF (Talk | contribs) m (shorten sentence) * (cur) (last) 18:47, 4 November 2006 WolfmanSF (Talk | contribs) m (Eliminate superfluous "However".) * (cur) (last) 18:38, 4 November 2006 WolfmanSF (Talk | contribs) (Revert to earlier version of this part of sentence.) * (cur) (last) 19:29, 19 August 2006 Hégésippe Cormier (Talk | contribs) m (+ interwikis) * (cur) (last) 06:28, 13 August 2006 WolfmanSF (Talk | contribs) (I point out that neutron degeneracy pressure is not the sole repulsive force supporting a neutron star against gravity (if it were, the TOV limit would be close to the Chandrasekhar limit).) * (cur) (last) 19:05, 25 July 2006 Irigi (Talk | contribs) m (+iw) * (cur) (last) 19:26, 8 June 2006 Christopher Thomas (Talk | contribs) m (Fixed run-on sentence.) * (cur) (last) 18:21, 8 June 2006 Nick Mks (Talk | contribs) (Stub indeed, but existing content is fine) * (cur) (last) 05:36, 6 June 2006 Tigerhawkvok (Talk | contribs) m * (cur) (last) 05:35, 6 June 2006 Tigerhawkvok (Talk | contribs) * (cur) (last) 07:26, 24 February 2006 Christopher Thomas (Talk | contribs) (Created stub article. References needed. Math and history would also be a plus.)
--GDK Δ 10:05, 11. Mai 2007 (CEST)
Es fehlt ein Wort.
Im Original heißt es: In an neutron star lighter than the limit, the weight of the star is supported by short-range repulsive neutron-neutron interactions mediated by the strong force and also the quantum degeneracy pressure of neutrons.
Bei der Übersetzung fehlt das Verb ("supported by"). Leider weiß ich nicht, wie man dies hier fachlich korrekt zu übersetzen hat.