FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2053829619> ?p ?o ?g. }

• W2053829619 endingPage "009" @default.
• W2053829619 startingPage "009" @default.
• W2053829619 abstract "The implications of the WMAP (Wilkinson Microwave Anisotropy Probe) third year data for inflation are investigated using both the slow-roll approximation and an exact numerical integration of the inflationary power spectra including a phenomenological modelling of the reheating era. At slow-roll leading order, the constraints 1 < 0.022 and −0.07 < 2 < 0.07 are obtained at the 95% CL (confidence level) implying a tensor to scalar ratio r10 < 0.21 and a Hubble parameter during inflation H/mPl < 1.3 × 10−5. At next-to-leading order, a tendency for 3 > 0 is observed. With regard to the exact numerical integration, large field models, , with p > 3.1 are now excluded at the 95% CL. Small field models, , are still compatible with the data for all values of p. However, if μ/mPl < 10 is assumed, then the case p = 2 is slightly disfavoured. In addition, mild constraints on the reheating temperature for an extreme equation of state are found, namely Treh > 2 TeV at the 95% CL. Hybrid models are disfavoured by the data, the best fit model having with two extra parameters in comparison with large field models. Running mass models remain compatible, but no prior independent constraints can be obtained. Finally, superimposed oscillations of trans-Planckian origin are studied. The vanilla slow-roll model is still the most probable one. However, the overall statistical weight in favour of superimposed oscillations has increased in comparison with the WMAP first year data, the amplitude of the oscillations satisfying 2|x|σ0 < 0.76 at the 95% CL. The best fit model leads to an improvement of for three extra parameters. Moreover, compared to other oscillatory patterns, the logarithmic shape is favoured." @default.
• W2053829619 created "2016-06-24" @default.
• W2053829619 creator A5047186097 @default.
• W2053829619 creator A5080651141 @default.
• W2053829619 date "2006-08-24" @default.
• W2053829619 modified "2023-10-14" @default.
• W2053829619 title "Inflation after WMAP3: confronting the slow-roll and exact power spectra with CMB data" @default.
• W2053829619 cites W1480081887 @default.
• W2053829619 cites W1537082240 @default.
• W2053829619 cites W1555237261 @default.
• W2053829619 cites W1572387126 @default.
• W2053829619 cites W1590390162 @default.
• W2053829619 cites W1669335760 @default.
• W2053829619 cites W1944901286 @default.
• W2053829619 cites W1964479029 @default.
• W2053829619 cites W1969293169 @default.
• W2053829619 cites W1971235146 @default.
• W2053829619 cites W1973861971 @default.
• W2053829619 cites W1974524768 @default.
• W2053829619 cites W1975247097 @default.
• W2053829619 cites W1977449087 @default.
• W2053829619 cites W1978881811 @default.
• W2053829619 cites W1980910499 @default.
• W2053829619 cites W1984165062 @default.
• W2053829619 cites W1985372504 @default.
• W2053829619 cites W1986717967 @default.
• W2053829619 cites W1999419759 @default.
• W2053829619 cites W2002374361 @default.
• W2053829619 cites W2004224441 @default.
• W2053829619 cites W2005276626 @default.
• W2053829619 cites W2011850528 @default.
• W2053829619 cites W2012869970 @default.
• W2053829619 cites W2012902029 @default.
• W2053829619 cites W2016298820 @default.
• W2053829619 cites W2017092488 @default.
• W2053829619 cites W2017143550 @default.
• W2053829619 cites W2018140428 @default.
• W2053829619 cites W2022354167 @default.
• W2053829619 cites W2025420969 @default.
• W2053829619 cites W2028201629 @default.
• W2053829619 cites W2030664362 @default.
• W2053829619 cites W2030987526 @default.
• W2053829619 cites W2033563716 @default.
• W2053829619 cites W2038096209 @default.
• W2053829619 cites W2039695817 @default.
• W2053829619 cites W2039916197 @default.
• W2053829619 cites W2043379579 @default.
• W2053829619 cites W2047568157 @default.
• W2053829619 cites W2047854232 @default.
• W2053829619 cites W2049038875 @default.
• W2053829619 cites W2056689787 @default.
• W2053829619 cites W2058194382 @default.
• W2053829619 cites W2058486682 @default.
• W2053829619 cites W2065692532 @default.
• W2053829619 cites W2066533993 @default.
• W2053829619 cites W2066796909 @default.
• W2053829619 cites W2067190132 @default.
• W2053829619 cites W2067502036 @default.
• W2053829619 cites W2069230998 @default.
• W2053829619 cites W2070953406 @default.
• W2053829619 cites W2074077513 @default.
• W2053829619 cites W2074752113 @default.
• W2053829619 cites W2075392245 @default.
• W2053829619 cites W2076847968 @default.
• W2053829619 cites W2077643264 @default.
• W2053829619 cites W2079765375 @default.
• W2053829619 cites W2081969560 @default.
• W2053829619 cites W2083387367 @default.
• W2053829619 cites W2083785101 @default.
• W2053829619 cites W2084137377 @default.
• W2053829619 cites W2090407220 @default.
• W2053829619 cites W2093463086 @default.
• W2053829619 cites W2093686531 @default.
• W2053829619 cites W2094806103 @default.
• W2053829619 cites W2096880613 @default.
• W2053829619 cites W2104239745 @default.
• W2053829619 cites W2106109252 @default.
• W2053829619 cites W2107918956 @default.
• W2053829619 cites W2108319641 @default.
• W2053829619 cites W2113544715 @default.
• W2053829619 cites W2125400604 @default.
• W2053829619 cites W2126294811 @default.
• W2053829619 cites W2133760636 @default.
• W2053829619 cites W2134251287 @default.
• W2053829619 cites W2144024295 @default.
• W2053829619 cites W2148534890 @default.
• W2053829619 cites W2148968450 @default.
• W2053829619 cites W2149699279 @default.
• W2053829619 cites W2149759149 @default.
• W2053829619 cites W2152900562 @default.
• W2053829619 cites W2153208487 @default.
• W2053829619 cites W2158442860 @default.
• W2053829619 cites W2160537828 @default.
• W2053829619 cites W2162550289 @default.
• W2053829619 cites W2169912865 @default.
• W2053829619 cites W2170963768 @default.
• W2053829619 cites W2174056583 @default.
• W2053829619 cites W2177467382 @default.

• next