On empty horizons in cosmological models
| ISSN: |
0375-9601
|
|---|---|
| Source: |
Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
|
| Topics: |
Physics
|
| Type of Medium: |
Electronic Resource
|
| URL: |
| _version_ | 1798291984263151618 |
|---|---|
| autor | King, A.R. |
| autorsonst | King, A.R. |
| book_url | http://linkinghub.elsevier.com/retrieve/pii/0375-9601(75)90830-0 |
| datenlieferant | nat_lic_papers |
| fussnote | The possibility that the matter density might become zero in certain regions of cosmological models is studied. It is shown that this can only occur in a non-singular way if the horizon is ''at infinity''. |
| hauptsatz | hsatz_simple |
| identnr | NLZ179291300 |
| issn | 0375-9601 |
| journal_name | Physics Letters A |
| materialart | 1 |
| package_name | Elsevier |
| publikationsort | Amsterdam |
| publisher | Elsevier |
| reference | 54 (1975), S. 115-116 |
| search_space | articles |
| shingle_author_1 | King, A.R. |
| shingle_author_2 | King, A.R. |
| shingle_author_3 | King, A.R. |
| shingle_author_4 | King, A.R. |
| shingle_catch_all_1 | King, A.R. On empty horizons in cosmological models 0375-9601 03759601 Elsevier |
| shingle_catch_all_2 | King, A.R. On empty horizons in cosmological models 0375-9601 03759601 Elsevier |
| shingle_catch_all_3 | King, A.R. On empty horizons in cosmological models 0375-9601 03759601 Elsevier |
| shingle_catch_all_4 | King, A.R. On empty horizons in cosmological models 0375-9601 03759601 Elsevier |
| shingle_title_1 | On empty horizons in cosmological models |
| shingle_title_2 | On empty horizons in cosmological models |
| shingle_title_3 | On empty horizons in cosmological models |
| shingle_title_4 | On empty horizons in cosmological models |
| sigel_instance_filter | dkfz geomar wilbert ipn albert fhp |
| source_archive | Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 |
| timestamp | 2024-05-06T08:41:18.627Z |
| titel | On empty horizons in cosmological models |
| titel_suche | On empty horizons in cosmological models The possibility that the matter density might become zero in certain regions of cosmological models is studied. It is shown that this can only occur in a non-singular way if the horizon is ''at infinity''. |
| topic | U |
| uid | nat_lic_papers_NLZ179291300 |