Dense matter in stellar collapse and neutron stars
In stellar collapse and neutron stars, matter reaches densities as high as an order of magnitude greater than that of nuclear matter. A review is given of the properties of nuclei in matter at sub-nuclear densities, a subject of importance for stellar collapse. Particular emphasis is placed on some...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1985 |
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| Reproduktion: |
Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 |
|---|---|
| Übergeordnetes Werk: |
in: Nuclear Physics, Section A - Amsterdam : Elsevier, 434(1985), Seite 587-604 |
| Übergeordnetes Werk: |
volume:434 ; year:1985 ; pages:587-604 |
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| 520 | |a In stellar collapse and neutron stars, matter reaches densities as high as an order of magnitude greater than that of nuclear matter. A review is given of the properties of nuclei in matter at sub-nuclear densities, a subject of importance for stellar collapse. Particular emphasis is placed on some of the very aspherical shapes nuclei can adopt. The properties of Skyrme's chiral soliton model at high densities, and the implications of the model for neutron stars and nuclear forces are discussed. | ||
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(DE-627)NLEJ181370247 (DE-599)GBVNLZ181370247 DE-627 ger DE-627 rakwb eng Dense matter in stellar collapse and neutron stars 1985 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier In stellar collapse and neutron stars, matter reaches densities as high as an order of magnitude greater than that of nuclear matter. A review is given of the properties of nuclei in matter at sub-nuclear densities, a subject of importance for stellar collapse. Particular emphasis is placed on some of the very aspherical shapes nuclei can adopt. The properties of Skyrme's chiral soliton model at high densities, and the implications of the model for neutron stars and nuclear forces are discussed. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Pethick, C.J. oth in Nuclear Physics, Section A Amsterdam : Elsevier 434(1985), Seite 587-604 (DE-627)NLEJ177217928 (DE-600)1466542-6 0375-9474 nnns volume:434 year:1985 pages:587-604 http://linkinghub.elsevier.com/retrieve/pii/0375-9474(85)90524-X GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 434 1985 587-604 |
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(DE-627)NLEJ181370247 (DE-599)GBVNLZ181370247 DE-627 ger DE-627 rakwb eng Dense matter in stellar collapse and neutron stars 1985 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier In stellar collapse and neutron stars, matter reaches densities as high as an order of magnitude greater than that of nuclear matter. A review is given of the properties of nuclei in matter at sub-nuclear densities, a subject of importance for stellar collapse. Particular emphasis is placed on some of the very aspherical shapes nuclei can adopt. The properties of Skyrme's chiral soliton model at high densities, and the implications of the model for neutron stars and nuclear forces are discussed. Elsevier Journal Backfiles on ScienceDirect 1907 - 2002 Pethick, C.J. oth in Nuclear Physics, Section A Amsterdam : Elsevier 434(1985), Seite 587-604 (DE-627)NLEJ177217928 (DE-600)1466542-6 0375-9474 nnns volume:434 year:1985 pages:587-604 http://linkinghub.elsevier.com/retrieve/pii/0375-9474(85)90524-X GBV_USEFLAG_H ZDB-1-SDJ GBV_NL_ARTICLE AR 434 1985 587-604 |
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Dense matter in stellar collapse and neutron stars |
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In stellar collapse and neutron stars, matter reaches densities as high as an order of magnitude greater than that of nuclear matter. A review is given of the properties of nuclei in matter at sub-nuclear densities, a subject of importance for stellar collapse. Particular emphasis is placed on some of the very aspherical shapes nuclei can adopt. The properties of Skyrme's chiral soliton model at high densities, and the implications of the model for neutron stars and nuclear forces are discussed. |
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In stellar collapse and neutron stars, matter reaches densities as high as an order of magnitude greater than that of nuclear matter. A review is given of the properties of nuclei in matter at sub-nuclear densities, a subject of importance for stellar collapse. Particular emphasis is placed on some of the very aspherical shapes nuclei can adopt. The properties of Skyrme's chiral soliton model at high densities, and the implications of the model for neutron stars and nuclear forces are discussed. |
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In stellar collapse and neutron stars, matter reaches densities as high as an order of magnitude greater than that of nuclear matter. A review is given of the properties of nuclei in matter at sub-nuclear densities, a subject of importance for stellar collapse. Particular emphasis is placed on some of the very aspherical shapes nuclei can adopt. The properties of Skyrme's chiral soliton model at high densities, and the implications of the model for neutron stars and nuclear forces are discussed. |
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