Can observations look back to the beginning of inflation?
The cosmic microwave background can measure the inflaton potential only if inflation lasts sufficiently long before the time of horizon crossing of observable fluctuations, such that non-linear effects in the time evolution of Green's functions lead to a loss of memory of initial conditions for...
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
15 January 2016
|
| In: |
Physics letters
Year: 2016, Jahrgang: 754, Pages: 109-113 |
| ISSN: | 1873-2445 |
| DOI: | 10.1016/j.physletb.2016.01.027 |
| Online-Zugang: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1016/j.physletb.2016.01.027 Verlag, lizenzpflichtig, Volltext: http://www.sciencedirect.com/science/article/pii/S0370269316000393 
|
| Verfasserangaben: | C. Wetterich |
MARC
| LEADER | 00000caa a2200000 c 4500 | ||
|---|---|---|---|
| 001 | 1724714406 | ||
| 003 | DE-627 | ||
| 005 | 20220818150510.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 200714s2016 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.1016/j.physletb.2016.01.027 |2 doi | |
| 035 | |a (DE-627)1724714406 | ||
| 035 | |a (DE-599)KXP1724714406 | ||
| 035 | |a (OCoLC)1341345119 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rda | ||
| 041 | |a eng | ||
| 084 | |a 29 |2 sdnb | ||
| 100 | 1 | |a Wetterich, Christof |d 1952- |e VerfasserIn |0 (DE-588)109400070 |0 (DE-627)683447629 |0 (DE-576)356552608 |4 aut | |
| 245 | 1 | 0 | |a Can observations look back to the beginning of inflation? |c C. Wetterich |
| 264 | 1 | |c 15 January 2016 | |
| 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 | ||
| 520 | |a The cosmic microwave background can measure the inflaton potential only if inflation lasts sufficiently long before the time of horizon crossing of observable fluctuations, such that non-linear effects in the time evolution of Green's functions lead to a loss of memory of initial conditions for the ultraviolet tail of the spectrum. Within a derivative expansion of the quantum effective action for an interacting scalar field we discuss the most general solution for the correlation function, including arbitrary pure and mixed quantum states. In this approximation no loss of memory occurs - cosmic microwave observations see the initial spectrum at the beginning of inflation, processed only mildly by the scale-violating effects at horizon crossing induced by the inflaton potential. | ||
| 773 | 0 | 8 | |i Enthalten in |t Physics letters |d Amsterdam : North-Holland Publ., 1967 |g 754(2016), Seite 109-113 |h Online-Ressource |w (DE-627)266015360 |w (DE-600)1466612-1 |w (DE-576)07495993X |x 1873-2445 |7 nnas |a Can observations look back to the beginning of inflation? |
| 773 | 1 | 8 | |g volume:754 |g year:2016 |g pages:109-113 |g extent:5 |a Can observations look back to the beginning of inflation? |
| 856 | 4 | 0 | |u https://doi.org/10.1016/j.physletb.2016.01.027 |x Verlag |x Resolving-System |z lizenzpflichtig |3 Volltext |
| 856 | 4 | 0 | |u http://www.sciencedirect.com/science/article/pii/S0370269316000393 |x Verlag |z lizenzpflichtig |3 Volltext |
| 951 | |a AR | ||
| 992 | |a 20200714 | ||
| 993 | |a Article | ||
| 994 | |a 2016 | ||
| 998 | |g 109400070 |a Wetterich, Christof |m 109400070:Wetterich, Christof |d 130000 |d 130300 |e 130000PW109400070 |e 130300PW109400070 |k 0/130000/ |k 1/130000/130300/ |p 1 |x j |y j | ||
| 999 | |a KXP-PPN1724714406 |e 3724252250 | ||
| BIB | |a Y | ||
| SER | |a journal | ||
| JSO | |a {"physDesc":[{"extent":"5 S."}],"type":{"bibl":"article-journal","media":"Online-Ressource"},"language":["eng"],"relHost":[{"physDesc":[{"extent":"Online-Ressource"}],"origin":[{"dateIssuedKey":"1967","publisher":"North-Holland Publ.","dateIssuedDisp":"1967-","publisherPlace":"Amsterdam"}],"id":{"issn":["1873-2445"],"zdb":["1466612-1"],"eki":["266015360"]},"type":{"media":"Online-Ressource","bibl":"periodical"},"disp":"Can observations look back to the beginning of inflation?Physics letters","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":{"extent":"5","text":"754(2016), Seite 109-113","volume":"754","pages":"109-113","year":"2016"},"title":[{"title":"Physics letters","title_sort":"Physics letters"}]}],"recId":"1724714406","name":{"displayForm":["C. Wetterich"]},"person":[{"family":"Wetterich","given":"Christof","roleDisplay":"VerfasserIn","display":"Wetterich, Christof","role":"aut"}],"origin":[{"dateIssuedDisp":"15 January 2016","dateIssuedKey":"2016"}],"title":[{"title_sort":"Can observations look back to the beginning of inflation?","title":"Can observations look back to the beginning of inflation?"}],"id":{"doi":["10.1016/j.physletb.2016.01.027"],"eki":["1724714406"]}} | ||
| SRT | |a WETTERICHCCANOBSERVA1520 | ||