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Titlebook: Historische Sinnbildung; Grundlagen, Formen, J?rn Rüsen Book 2020 Springer Fachmedien Wiesbaden GmbH, ein Teil von Springer Nature 2020 Si

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發(fā)表于 2025-3-25 04:33:20 | 只看該作者
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發(fā)表于 2025-3-25 15:26:34 | 只看該作者
J?rn Rüseno derive the expressions for the energy loss due to ultra light scalars and vector bosons from binary stars. The direct observation of gravitational waves by Ligo and Virgo from black hole and neutrons star merger was a landmark evert which has opened the area of multi-messenger astronomy. In this c
24#
發(fā)表于 2025-3-25 18:51:14 | 只看該作者
J?rn Rüseneriments. The second part discusses the production of neutrinos by interactions of the primary cosmic rays both within the sources and during propagation from the source to the observer, along with the resulting neutrino fluxes. Figure?. summarizes the diffuse “grand unified” neutrino spectrum exten
25#
發(fā)表于 2025-3-25 23:57:17 | 只看該作者
J?rn Rüseneriments. The second part discusses the production of neutrinos by interactions of the primary cosmic rays both within the sources and during propagation from the source to the observer, along with the resulting neutrino fluxes. Figure?. summarizes the diffuse “grand unified” neutrino spectrum exten
26#
發(fā)表于 2025-3-26 03:17:32 | 只看該作者
J?rn Rüseneriments. The second part discusses the production of neutrinos by interactions of the primary cosmic rays both within the sources and during propagation from the source to the observer, along with the resulting neutrino fluxes. Figure?. summarizes the diffuse “grand unified” neutrino spectrum exten
27#
發(fā)表于 2025-3-26 05:55:15 | 只看該作者
28#
發(fā)表于 2025-3-26 12:27:44 | 只看該作者
J?rn Rüsenpically in phase transitions which in turn are often associated with the breaking of symmetries of interactions. Such phase transitions can leave primordial relics such as magnetic fields and small excesses of lepton and baryon number as we see them today which is developed next. The following two s
29#
發(fā)表于 2025-3-26 14:47:35 | 只看該作者
J?rn Rüsen rates and propagation, the first part focuses on propagation within our Galaxy which is dominated by diffusive processes. Interactions and energy losses are generally more prominent for propagation over extragalactic distances, which is the subject of the second part. The propagation of high energy
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發(fā)表于 2025-3-26 17:29:50 | 只看該作者
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