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| 001 | 289123 | ||
| 005 | 20211110132541.0 | ||
| 037 | _ | _ | |a PUBDB-2015-05250 |
| 100 | 1 | _ | |a Broy, Benedict |0 P:(DE-H253)PIP1018435 |b 0 |e Corresponding author |
| 245 | _ | _ | |a Starobinsky-Type Inflation |
| 260 | _ | _ | |c 2015 |
| 336 | 7 | _ | |a Talk (non-conference) |b talk |m talk |0 PUB:(DE-HGF)31 |s 1449582142_25279 |2 PUB:(DE-HGF) |x Seminar Talk |
| 336 | 7 | _ | |a Conference Paper |0 33 |2 EndNote |
| 336 | 7 | _ | |a Other |2 DINI |
| 336 | 7 | _ | |a INPROCEEDINGS |2 BibTeX |
| 502 | _ | _ | |c Groningen U |
| 520 | _ | _ | |a Both WMAP and PLANCK have hinted at a slight suppression of power in the CMB temperature spectrum at large angular scales. Yet this power loss is usually unaccounted for by models that are claimed to provide a best fit to the data at first order, such as the Starobinsky f(R) model. In a first step, we demonstrate how to obtain a viable observational signature in f(R) theory by explicitly constructing higher order terms to the Starobinsky model. In a second step, we outline a new inflationary scenario deriving from higher derivative corrections in String theory giving rise to a similar observational fingerprint. |
| 536 | _ | _ | |0 G:(DE-HGF)POF3-611 |c POF3-611 |f POF III |x 0 |a 611 - Fundamental Particles and Forces (POF3-611) |
| 536 | _ | _ | |0 G:(DE-HGF)2015_IFV-HZ-NG-603 |x 1 |c 2015_IFV-HZ-NG-603 |a HZ-NG-603 - Strings and Cosmology - an Interface for Testing fundamental Theories (2015_IFV-HZ-NG-603) |
| 693 | _ | _ | |0 EXP:(DE-MLZ)NOSPEC-20140101 |5 EXP:(DE-MLZ)NOSPEC-20140101 |e No specific instrument |x 0 |
| 856 | 4 | _ | |u https://bib-pubdb1.desy.de/record/289123/files/Talk.pdf |y OpenAccess |
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| 914 | 1 | _ | |y 2015 |
| 915 | _ | _ | |a OpenAccess |0 StatID:(DE-HGF)0510 |2 StatID |
| 920 | 1 | _ | |0 I:(DE-H253)T-20120731 |k T |l Theorie-Gruppe |x 0 |
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| 980 | _ | _ | |a talk |
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| 980 | _ | _ | |a UNRESTRICTED |
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