Three-form cosmology
Cosmology of self-interacting three-forms is investigated. The minimally coupled canonical theory can naturally generate a variety of isotropic background dynamics, including scaling, possibly transient acceleration and phantom crossing. An intuitive picture of the cosmological dynamics is presented...
Gespeichert in:
| Hauptverfasser: | , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
26 January 2010
|
| In: |
Physics letters
Year: 2010, Jahrgang: 685, Heft: 2, Pages: 105-109 |
| ISSN: | 1873-2445 |
| DOI: | 10.1016/j.physletb.2010.01.051 |
| Online-Zugang: | Resolving-System, lizenzpflichtig, Volltext: https://doi.org/10.1016/j.physletb.2010.01.051 Verlag, lizenzpflichtig, Volltext: https://www.sciencedirect.com/science/article/pii/S0370269310001097 |
| Verfasserangaben: | Tomi S. Koivisto, Nelson J. Nunes |
MARC
| LEADER | 00000caa a2200000 c 4500 | ||
|---|---|---|---|
| 001 | 1839644591 | ||
| 003 | DE-627 | ||
| 005 | 20230710145845.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 230321s2010 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.1016/j.physletb.2010.01.051 |2 doi | |
| 035 | |a (DE-627)1839644591 | ||
| 035 | |a (DE-599)KXP1839644591 | ||
| 035 | |a (OCoLC)1389807130 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rda | ||
| 041 | |a eng | ||
| 084 | |a 29 |2 sdnb | ||
| 100 | 1 | |a Koivisto, Tomi |e VerfasserIn |0 (DE-588)1283953587 |0 (DE-627)183964558X |4 aut | |
| 245 | 1 | 0 | |a Three-form cosmology |c Tomi S. Koivisto, Nelson J. Nunes |
| 264 | 1 | |c 26 January 2010 | |
| 300 | |a 5 | ||
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a Computermedien |b c |2 rdamedia | ||
| 338 | |a Online-Ressource |b cr |2 rdacarrier | ||
| 500 | |a Gesehen am 21.03.2023 | ||
| 520 | |a Cosmology of self-interacting three-forms is investigated. The minimally coupled canonical theory can naturally generate a variety of isotropic background dynamics, including scaling, possibly transient acceleration and phantom crossing. An intuitive picture of the cosmological dynamics is presented employing an effective potential. Numerical solutions and analytical approximations are provided for scenarios which are potentially important for inflation or dark energy. | ||
| 650 | 4 | |a -forms | |
| 650 | 4 | |a Cosmology | |
| 650 | 4 | |a Dark energy | |
| 650 | 4 | |a Inflation | |
| 650 | 4 | |a Theory | |
| 700 | 1 | |a Nunes, Nelson |e VerfasserIn |0 (DE-588)104730953X |0 (DE-627)778095738 |0 (DE-576)358994551 |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Physics letters |d Amsterdam : North-Holland Publ., 1967 |g 685(2010), 2, Seite 105-109 |h Online-Ressource |w (DE-627)266015360 |w (DE-600)1466612-1 |w (DE-576)07495993X |x 1873-2445 |7 nnas |a Three-form cosmology |
| 773 | 1 | 8 | |g volume:685 |g year:2010 |g number:2 |g pages:105-109 |g extent:5 |a Three-form cosmology |
| 856 | 4 | 0 | |u https://doi.org/10.1016/j.physletb.2010.01.051 |x Resolving-System |x Verlag |z lizenzpflichtig |3 Volltext |
| 856 | 4 | 0 | |u https://www.sciencedirect.com/science/article/pii/S0370269310001097 |x Verlag |z lizenzpflichtig |3 Volltext |
| 951 | |a AR | ||
| 992 | |a 20230321 | ||
| 993 | |a Article | ||
| 994 | |a 2010 | ||
| 998 | |g 104730953X |a Nunes, Nelson |m 104730953X:Nunes, Nelson |d 130000 |d 130300 |e 130000PN104730953X |e 130300PN104730953X |k 0/130000/ |k 1/130000/130300/ |p 2 |y j | ||
| 998 | |g 1283953587 |a Koivisto, Tomi |m 1283953587:Koivisto, Tomi |d 130000 |d 130300 |e 130000PK1283953587 |e 130300PK1283953587 |k 0/130000/ |k 1/130000/130300/ |p 1 |x j | ||
| 999 | |a KXP-PPN1839644591 |e 4293968822 | ||
| BIB | |a Y | ||
| SER | |a journal | ||
| JSO | |a {"physDesc":[{"extent":"5 S."}],"relHost":[{"origin":[{"dateIssuedKey":"1967","publisher":"North-Holland Publ.","dateIssuedDisp":"1967-","publisherPlace":"Amsterdam"}],"id":{"eki":["266015360"],"zdb":["1466612-1"],"issn":["1873-2445"]},"physDesc":[{"extent":"Online-Ressource"}],"title":[{"title":"Physics letters","title_sort":"Physics letters"}],"disp":"Three-form cosmologyPhysics letters","type":{"bibl":"periodical","media":"Online-Ressource"},"note":["Gesehen am 24.06.24","Fortsetzung der Druck-Ausgabe","Ab 2014 mit durchgehender Heftzählung, die als Vol. bez. wird"],"language":["eng"],"recId":"266015360","pubHistory":["24.1967 - 727.2013; Vol. 728.2014 -"],"titleAlt":[{"title":"Physics letters / B"}],"part":{"volume":"685","text":"685(2010), 2, Seite 105-109","extent":"5","year":"2010","issue":"2","pages":"105-109"}}],"origin":[{"dateIssuedDisp":"26 January 2010","dateIssuedKey":"2010"}],"id":{"doi":["10.1016/j.physletb.2010.01.051"],"eki":["1839644591"]},"name":{"displayForm":["Tomi S. Koivisto, Nelson J. Nunes"]},"note":["Gesehen am 21.03.2023"],"type":{"media":"Online-Ressource","bibl":"article-journal"},"language":["eng"],"recId":"1839644591","title":[{"title":"Three-form cosmology","title_sort":"Three-form cosmology"}],"person":[{"family":"Koivisto","given":"Tomi","display":"Koivisto, Tomi","roleDisplay":"VerfasserIn","role":"aut"},{"role":"aut","roleDisplay":"VerfasserIn","display":"Nunes, Nelson","given":"Nelson","family":"Nunes"}]} | ||
| SRT | |a KOIVISTOTOTHREEFORMC2620 | ||