Baryonic Dark Matter:
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1990
|
| Schriftenreihe: | NATO ASI Series, Series C: Mathematical and Physical Sciences
306 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | The visible universe is a small perturbation on the material universe. Zwicky and Sinclair Smith in the 1930s gave evidence of invisible mass in the Coma and Virgo Clusters of Galaxies. Better optical data has only served to confound their critics and the X-ray data confirms that the gravitational potentials are many times larger than those predicted on the basis of the observed stars. Dynamical analyses of individual galaxies have found that significant extra mass is needed to explain their rotational velocities. On much larger scales, tens of megaparsecs, there is suggestive evidence that there is even more mass per unit luminosity. What is this non-luminous stuff of which the universe is made'? How much of it is there? Need there be only one kind of stuff? There are three basic possi bili ties:- all of it is ordinary (baryonic) matter, all of it is some other kind of (non-baryonic) matter, or some of it is baryonic and some is non-baryonic |
| Beschreibung: | 1 Online-Ressource (XII, 298 p) |
| ISBN: | 9789400905658 9789401067423 |
| ISSN: | 1389-2185 |
| DOI: | 10.1007/978-94-009-0565-8 |
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| 245 | 1 | 0 | |a Baryonic Dark Matter |c edited by D. Lynden-Bell, G. Gilmore |
| 246 | 1 | 3 | |a Proceedings of the NATO Advanced Study Institute, Cambridge, U.K., July 17-28, 1989 |
| 264 | 1 | |a Dordrecht |b Springer Netherlands |c 1990 | |
| 300 | |a 1 Online-Ressource (XII, 298 p) | ||
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| 500 | |a The visible universe is a small perturbation on the material universe. Zwicky and Sinclair Smith in the 1930s gave evidence of invisible mass in the Coma and Virgo Clusters of Galaxies. Better optical data has only served to confound their critics and the X-ray data confirms that the gravitational potentials are many times larger than those predicted on the basis of the observed stars. Dynamical analyses of individual galaxies have found that significant extra mass is needed to explain their rotational velocities. On much larger scales, tens of megaparsecs, there is suggestive evidence that there is even more mass per unit luminosity. What is this non-luminous stuff of which the universe is made'? How much of it is there? Need there be only one kind of stuff? There are three basic possi bili ties:- all of it is ordinary (baryonic) matter, all of it is some other kind of (non-baryonic) matter, or some of it is baryonic and some is non-baryonic | ||
| 650 | 4 | |a Physics | |
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Datensatz im Suchindex
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| author | Lynden-Bell, D. |
| author_facet | Lynden-Bell, D. |
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| author_sort | Lynden-Bell, D. |
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| bvnumber | BV042414906 |
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| dewey-full | 530.1 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 530 - Physics |
| dewey-raw | 530.1 |
| dewey-search | 530.1 |
| dewey-sort | 3530.1 |
| dewey-tens | 530 - Physics |
| discipline | Physik |
| doi_str_mv | 10.1007/978-94-009-0565-8 |
| format | Electronic eBook |
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| spelling | Lynden-Bell, D. Verfasser aut Baryonic Dark Matter edited by D. Lynden-Bell, G. Gilmore Proceedings of the NATO Advanced Study Institute, Cambridge, U.K., July 17-28, 1989 Dordrecht Springer Netherlands 1990 1 Online-Ressource (XII, 298 p) txt rdacontent c rdamedia cr rdacarrier NATO ASI Series, Series C: Mathematical and Physical Sciences 306 1389-2185 The visible universe is a small perturbation on the material universe. Zwicky and Sinclair Smith in the 1930s gave evidence of invisible mass in the Coma and Virgo Clusters of Galaxies. Better optical data has only served to confound their critics and the X-ray data confirms that the gravitational potentials are many times larger than those predicted on the basis of the observed stars. Dynamical analyses of individual galaxies have found that significant extra mass is needed to explain their rotational velocities. On much larger scales, tens of megaparsecs, there is suggestive evidence that there is even more mass per unit luminosity. What is this non-luminous stuff of which the universe is made'? How much of it is there? Need there be only one kind of stuff? There are three basic possi bili ties:- all of it is ordinary (baryonic) matter, all of it is some other kind of (non-baryonic) matter, or some of it is baryonic and some is non-baryonic Physics Classical and Quantum Gravitation, Relativity Theory Astronomy, Observations and Techniques Astrophysics and Astroparticles Schwarzes Loch (DE-588)4053793-6 gnd rswk-swf Baryon (DE-588)4144076-6 gnd rswk-swf 1\p (DE-588)1071861417 Konferenzschrift 1989 Cambridge gnd-content Schwarzes Loch (DE-588)4053793-6 s Baryon (DE-588)4144076-6 s 2\p DE-604 Gilmore, G. Sonstige oth https://doi.org/10.1007/978-94-009-0565-8 Verlag Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk 2\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Lynden-Bell, D. Baryonic Dark Matter Physics Classical and Quantum Gravitation, Relativity Theory Astronomy, Observations and Techniques Astrophysics and Astroparticles Schwarzes Loch (DE-588)4053793-6 gnd Baryon (DE-588)4144076-6 gnd |
| subject_GND | (DE-588)4053793-6 (DE-588)4144076-6 (DE-588)1071861417 |
| title | Baryonic Dark Matter |
| title_alt | Proceedings of the NATO Advanced Study Institute, Cambridge, U.K., July 17-28, 1989 |
| title_auth | Baryonic Dark Matter |
| title_exact_search | Baryonic Dark Matter |
| title_full | Baryonic Dark Matter edited by D. Lynden-Bell, G. Gilmore |
| title_fullStr | Baryonic Dark Matter edited by D. Lynden-Bell, G. Gilmore |
| title_full_unstemmed | Baryonic Dark Matter edited by D. Lynden-Bell, G. Gilmore |
| title_short | Baryonic Dark Matter |
| title_sort | baryonic dark matter |
| topic | Physics Classical and Quantum Gravitation, Relativity Theory Astronomy, Observations and Techniques Astrophysics and Astroparticles Schwarzes Loch (DE-588)4053793-6 gnd Baryon (DE-588)4144076-6 gnd |
| topic_facet | Physics Classical and Quantum Gravitation, Relativity Theory Astronomy, Observations and Techniques Astrophysics and Astroparticles Schwarzes Loch Baryon Konferenzschrift 1989 Cambridge |
| url | https://doi.org/10.1007/978-94-009-0565-8 |
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