Matches in SemOpenAlex for { <https://semopenalex.org/work/W1993663358> ?p ?o ?g. }
- W1993663358 endingPage "533" @default.
- W1993663358 startingPage "525" @default.
- W1993663358 abstract "We reassess constraints on the cosmological baryon density from observations of the mean decrement and power spectrum of the Lyα forest, taking into account uncertainties in all free parameters in the simplest gravitational instability model. The uncertainty is dominated by that of the photoionizing background, but incomplete knowledge of the thermal state of the intergalactic medium also contributes significantly to the error budget. While current estimates of the baryon fraction from the forest do prefer values that are somewhat higher than the big bang nucleosynthesis value of Ωb h2 = 0.02 ± 0.001, the discrepancy is at most about 3 σ. For instance, assuming the highest estimate of the ionizing background, as indicated by recent measurements of a large escape fraction from Lyman break galaxies by Steidel, Pettini, & Adelberger, we find Ωbh2 = 0.045 ± 0.008. A recent measurement of the ionizing background from the proximity effect by Scott et al., on the other hand, implies Ωbh2 = 0.03 ± 0.01. We provide an expression from which future likelihoods for Ωb h2 can be derived as measurements of the ionizing background improve—consistency among constraints from the forest, nucleosynthesis, and the microwave background will provide a powerful test of the gravitational instability model for the forest and for large-scale structure in general. We also develop a formalism that treats lower bounds on the baryon density in a statistical manner, which is appropriate if only a lower bound on the ionizing background is known. Finally, we discuss the implications of the escape fraction measurement for the age, structure, and stellar content of Lyman break galaxies. We show that the observed hard spectrum from Lyman break galaxies requires a very young age (less than about 1 million years) and/or a top-heavy initial mass function. We also build a model in which an extended (non-disk-like) gas distribution allows a large escape fraction." @default.
- W1993663358 created "2016-06-24" @default.
- W1993663358 creator A5024721944 @default.
- W1993663358 creator A5036506366 @default.
- W1993663358 creator A5085339462 @default.
- W1993663358 creator A5089500886 @default.
- W1993663358 date "2002-01-10" @default.
- W1993663358 modified "2023-09-28" @default.
- W1993663358 title "Connections between the Cosmic Baryon Fraction, the Extragalactic Ionizing Background, and Lyman Break Galaxies" @default.
- W1993663358 cites W1486486469 @default.
- W1993663358 cites W1487093425 @default.
- W1993663358 cites W1534059466 @default.
- W1993663358 cites W1566749576 @default.
- W1993663358 cites W1908017297 @default.
- W1993663358 cites W1965439243 @default.
- W1993663358 cites W1971204277 @default.
- W1993663358 cites W1979588734 @default.
- W1993663358 cites W2006869439 @default.
- W1993663358 cites W2011663358 @default.
- W1993663358 cites W2018950554 @default.
- W1993663358 cites W2021494017 @default.
- W1993663358 cites W2023122552 @default.
- W1993663358 cites W2025187234 @default.
- W1993663358 cites W2029566685 @default.
- W1993663358 cites W2035877537 @default.
- W1993663358 cites W2037351399 @default.
- W1993663358 cites W2037624693 @default.
- W1993663358 cites W2039652706 @default.
- W1993663358 cites W2043546334 @default.
- W1993663358 cites W2050684496 @default.
- W1993663358 cites W2054755664 @default.
- W1993663358 cites W2057702826 @default.
- W1993663358 cites W2059079350 @default.
- W1993663358 cites W2059511259 @default.
- W1993663358 cites W2061402667 @default.
- W1993663358 cites W2075740186 @default.
- W1993663358 cites W2080312273 @default.
- W1993663358 cites W2080845713 @default.
- W1993663358 cites W2083472313 @default.
- W1993663358 cites W2086248392 @default.
- W1993663358 cites W2090877402 @default.
- W1993663358 cites W2091008984 @default.
- W1993663358 cites W2092618688 @default.
- W1993663358 cites W2106285612 @default.
- W1993663358 cites W2114951275 @default.
- W1993663358 cites W2125603062 @default.
- W1993663358 cites W2137982811 @default.
- W1993663358 cites W2141421120 @default.
- W1993663358 cites W2143951133 @default.
- W1993663358 cites W2156913827 @default.
- W1993663358 cites W2599720466 @default.
- W1993663358 cites W2952332536 @default.
- W1993663358 cites W3097983063 @default.
- W1993663358 cites W3098144429 @default.
- W1993663358 cites W3098654032 @default.
- W1993663358 cites W3100010580 @default.
- W1993663358 cites W3100110286 @default.
- W1993663358 cites W3100195711 @default.
- W1993663358 cites W3100401081 @default.
- W1993663358 cites W3100810381 @default.
- W1993663358 cites W3101168514 @default.
- W1993663358 cites W3101649655 @default.
- W1993663358 cites W3101697479 @default.
- W1993663358 cites W3102056806 @default.
- W1993663358 cites W3102763870 @default.
- W1993663358 cites W3104344646 @default.
- W1993663358 cites W3104416848 @default.
- W1993663358 cites W3105115771 @default.
- W1993663358 cites W3105778198 @default.
- W1993663358 cites W3106124635 @default.
- W1993663358 cites W3124780147 @default.
- W1993663358 cites W4244818491 @default.
- W1993663358 doi "https://doi.org/10.1086/324401" @default.
- W1993663358 hasPublicationYear "2002" @default.
- W1993663358 type Work @default.
- W1993663358 sameAs 1993663358 @default.
- W1993663358 citedByCount "21" @default.
- W1993663358 crossrefType "journal-article" @default.
- W1993663358 hasAuthorship W1993663358A5024721944 @default.
- W1993663358 hasAuthorship W1993663358A5036506366 @default.
- W1993663358 hasAuthorship W1993663358A5085339462 @default.
- W1993663358 hasAuthorship W1993663358A5089500886 @default.
- W1993663358 hasBestOaLocation W19936633581 @default.
- W1993663358 hasConcept C121332964 @default.
- W1993663358 hasConcept C127592171 @default.
- W1993663358 hasConcept C1276947 @default.
- W1993663358 hasConcept C154153549 @default.
- W1993663358 hasConcept C16743098 @default.
- W1993663358 hasConcept C207297109 @default.
- W1993663358 hasConcept C26405456 @default.
- W1993663358 hasConcept C2993745857 @default.
- W1993663358 hasConcept C33024259 @default.
- W1993663358 hasConcept C4397270 @default.
- W1993663358 hasConcept C44870925 @default.
- W1993663358 hasConcept C62520636 @default.
- W1993663358 hasConcept C62796785 @default.
- W1993663358 hasConcept C69672822 @default.
- W1993663358 hasConcept C85725439 @default.