Supernova legacy survey data are consistent with acceleration at z [approximately-equal sign] 3
We point out that the Type Ia supernovae in the SNLS dataset are consistent with an early beginning of the cosmic acceleration if dark energy interacts strongly with dark matter. We find that the acceleration could have started at redshift z≈3 and higher.
Saved in:
| Main Authors: | , , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
12 December 2006
|
| In: |
Physical review. D, Particles, fields, gravitation, and cosmology
Year: 2006, Volume: 74, Issue: 12, Pages: 127302 |
| ISSN: | 1550-2368 |
| DOI: | 10.1103/PhysRevD.74.127302 |
| Online Access: | Verlag, Volltext: http://dx.doi.org/10.1103/PhysRevD.74.127302 Verlag, Volltext: https://link.aps.org/doi/10.1103/PhysRevD.74.127302 
|
| Author Notes: | Luca Amendola, M. Gasperini, and Federico Piazza |
MARC
| LEADER | 00000caa a2200000 c 4500 | ||
|---|---|---|---|
| 001 | 1565369661 | ||
| 003 | DE-627 | ||
| 005 | 20220814022709.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 171115s2006 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.1103/PhysRevD.74.127302 |2 doi | |
| 035 | |a (DE-627)1565369661 | ||
| 035 | |a (DE-576)495369667 | ||
| 035 | |a (DE-599)BSZ495369667 | ||
| 035 | |a (OCoLC)1340981734 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rda | ||
| 041 | |a eng | ||
| 084 | |a 29 |2 sdnb | ||
| 100 | 1 | |a Amendola, Luca |d 1963- |e VerfasserIn |0 (DE-588)1029171270 |0 (DE-627)732547482 |0 (DE-576)377045128 |4 aut | |
| 245 | 1 | 0 | |a Supernova legacy survey data are consistent with acceleration at z [approximately-equal sign] 3 |c Luca Amendola, M. Gasperini, and Federico Piazza |
| 246 | 3 | 0 | |a z ≈ 3 z≈3 |
| 264 | 1 | |c 12 December 2006 | |
| 300 | |a 3 | ||
| 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 15.11.2017 | ||
| 520 | |a We point out that the Type Ia supernovae in the SNLS dataset are consistent with an early beginning of the cosmic acceleration if dark energy interacts strongly with dark matter. We find that the acceleration could have started at redshift z≈3 and higher. | ||
| 700 | 1 | |a Gasperini, Maurizio |d 1952- |e VerfasserIn |0 (DE-588)133861783 |0 (DE-627)557857430 |0 (DE-576)301552703 |4 aut | |
| 700 | 1 | |a Piazza, Federico |e VerfasserIn |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Physical review. D, Particles, fields, gravitation, and cosmology |d [Erscheinungsort nicht ermittelbar] : Soc., 1970 |g 74(2006,12) Artikel-Nummer 127302, 3 Seiten |h Online-Ressource |w (DE-627)253787017 |w (DE-600)1461167-3 |w (DE-576)07279531X |x 1550-2368 |7 nnas |a Supernova legacy survey data are consistent with acceleration at z [approximately-equal sign] 3 |
| 773 | 1 | 8 | |g volume:74 |g year:2006 |g number:12 |g pages:127302 |g extent:3 |a Supernova legacy survey data are consistent with acceleration at z [approximately-equal sign] 3 |
| 856 | 4 | 0 | |u http://dx.doi.org/10.1103/PhysRevD.74.127302 |x Verlag |x Resolving-System |3 Volltext |
| 856 | 4 | 0 | |u https://link.aps.org/doi/10.1103/PhysRevD.74.127302 |x Verlag |3 Volltext |
| 951 | |a AR | ||
| 992 | |a 20171115 | ||
| 993 | |a Article | ||
| 994 | |a 2006 | ||
| 998 | |g 1029171270 |a Amendola, Luca |m 1029171270:Amendola, Luca |p 1 |x j | ||
| 999 | |a KXP-PPN1565369661 |e 2987232675 | ||
| BIB | |a Y | ||
| SER | |a journal | ||
| JSO | |a {"note":["Gesehen am 15.11.2017"],"recId":"1565369661","name":{"displayForm":["Luca Amendola, M. Gasperini, and Federico Piazza"]},"origin":[{"dateIssuedKey":"2006","dateIssuedDisp":"12 December 2006"}],"person":[{"display":"Amendola, Luca","role":"aut","family":"Amendola","given":"Luca"},{"display":"Gasperini, Maurizio","role":"aut","family":"Gasperini","given":"Maurizio"},{"family":"Piazza","given":"Federico","display":"Piazza, Federico","role":"aut"}],"language":["eng"],"title":[{"title_sort":"Supernova legacy survey data are consistent with acceleration at z [approximately-equal sign] 3","title":"Supernova legacy survey data are consistent with acceleration at z [approximately-equal sign] 3"}],"relHost":[{"language":["eng"],"title":[{"title":"Physical review","partname":"Particles, fields, gravitation, and cosmology","title_sort":"Physical review"}],"physDesc":[{"extent":"Online-Ressource"}],"note":["ISSN-Portal 1089-4918: Particles and fields","Gesehen am 22. Januar 2016"],"disp":"Supernova legacy survey data are consistent with acceleration at z [approximately-equal sign] 3Physical review. D, Particles, fields, gravitation, and cosmology","name":{"displayForm":["publ. by the American Physical Society through the American Institute of Physics"]},"corporate":[{"role":"isb","display":"American Institute of Physics"},{"role":"isb","display":"American Physical Society"}],"pubHistory":["3.Ser. 1.1970 - 92.2015"],"part":{"pages":"127302","issue":"12","text":"74(2006,12) Artikel-Nummer 127302, 3 Seiten","volume":"74","year":"2006","extent":"3"},"id":{"issn":["1550-2368","1089-4918"],"zdb":["1461167-3"],"eki":["253787017"]},"type":{"bibl":"periodical","media":"Online-Ressource"},"recId":"253787017","titleAlt":[{"title":"Physical review / D"},{"title":"D online"}],"origin":[{"publisherPlace":"[Erscheinungsort nicht ermittelbar]","dateIssuedKey":"1970","dateIssuedDisp":"1970-2015","publisher":"Soc."}]}],"physDesc":[{"extent":"3 S."}],"id":{"eki":["1565369661"],"doi":["10.1103/PhysRevD.74.127302"]},"type":{"media":"Online-Ressource","bibl":"article-journal"}} | ||
| SRT | |a AMENDOLALUSUPERNOVAL1220 | ||