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000289123 1001_ $$0P:(DE-H253)PIP1018435$$aBroy, Benedict$$b0$$eCorresponding author
000289123 245__ $$aStarobinsky-Type Inflation
000289123 260__ $$c2015
000289123 3367_ $$0PUB:(DE-HGF)31$$2PUB:(DE-HGF)$$aTalk (non-conference)$$btalk$$mtalk$$s1449582142_25279$$xSeminar Talk
000289123 3367_ $$033$$2EndNote$$aConference Paper
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000289123 3367_ $$2BibTeX$$aINPROCEEDINGS
000289123 502__ $$cGroningen U
000289123 520__ $$aBoth 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.
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000289123 536__ $$0G:(DE-HGF)2015_IFV-HZ-NG-603$$aHZ-NG-603 - Strings and Cosmology - an Interface for Testing fundamental Theories (2015_IFV-HZ-NG-603)$$c2015_IFV-HZ-NG-603$$x1
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000289123 9141_ $$y2015
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