FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2127497500> ?p ?o ?g. }

• W2127497500 endingPage "113" @default.
• W2127497500 startingPage "96" @default.
• W2127497500 abstract "Cosmological expansion cannot produce the reported correlations of the gamma-ray burst timescale and spectral energy with peak flux if the burst model reproduces the Burst and Transient Source Experiment (BATSE) 3B peak flux distribution for a nonevolving burst source density. The required ratios of time dilation and redshift factors are only produced by monoluminous models at peak fluxes below the BATSE threshold, and they are never produced by power-law luminosity models. Monoluminous models produce acceptable fits to the peak flux distribution only for very specific combinations of the spectral and cosmological parameters. The redshift of gamma-ray bursts at the BATSE threshold is z ≈ 1.5. Power-law luminosity distribution models ∝L-β produce acceptable fits to the data for most values of the spectral parameters when β < 1.6. In this model, gamma-ray bursts of a given peak flux have a distribution of redshifts, with a maximum redshift of ≳3 for peak fluxes near the BATSE threshold and with an average redshift of <1 for all values of peak flux. This qualitative behavior occurs whenever the luminosity distribution determines the shape of the peak flux distribution, regardless of whether source density evolution occurs. The reported correlations of the burst timescale and the spectral energy with peak flux are systematically 1 standard deviation above the monoluminous model and 1.5-2 standard deviations above the power-law luminosity model. These results suggest that an intrinsic correlation of burst timescale and spectral energy with luminosity is present. Studies of the peak flux distribution for bursts selected by Epeak or the hardness ratio provide a test for this intrinsic correlation." @default.
• W2127497500 created "2016-06-24" @default.
• W2127497500 creator A5061902661 @default.
• W2127497500 date "1997-09-20" @default.
• W2127497500 modified "2023-09-26" @default.
• W2127497500 title "The Cosmological Signatures and Flux Distribution of Gamma‐Ray Bursts with a Broad Luminosity Distribution" @default.
• W2127497500 cites W1504372976 @default.
• W2127497500 cites W1543600439 @default.
• W2127497500 cites W1575795934 @default.
• W2127497500 cites W1653673423 @default.
• W2127497500 cites W1661808469 @default.
• W2127497500 cites W1965500901 @default.
• W2127497500 cites W1974602111 @default.
• W2127497500 cites W1986586747 @default.
• W2127497500 cites W1988406600 @default.
• W2127497500 cites W2010051090 @default.
• W2127497500 cites W2014036427 @default.
• W2127497500 cites W2019518795 @default.
• W2127497500 cites W2021157451 @default.
• W2127497500 cites W2021636649 @default.
• W2127497500 cites W2029660793 @default.
• W2127497500 cites W2031906877 @default.
• W2127497500 cites W2050543292 @default.
• W2127497500 cites W2067148104 @default.
• W2127497500 cites W2078266217 @default.
• W2127497500 cites W2080583435 @default.
• W2127497500 cites W2080810614 @default.
• W2127497500 cites W2081856580 @default.
• W2127497500 cites W2090017763 @default.
• W2127497500 cites W2092218241 @default.
• W2127497500 cites W2997052184 @default.
• W2127497500 cites W2997412783 @default.
• W2127497500 cites W3098412624 @default.
• W2127497500 cites W3098650997 @default.
• W2127497500 cites W3098847322 @default.
• W2127497500 cites W3099379667 @default.
• W2127497500 cites W3100857035 @default.
• W2127497500 cites W3102065493 @default.
• W2127497500 cites W3105902394 @default.
• W2127497500 cites W3105329975 @default.
• W2127497500 doi "https://doi.org/10.1086/304585" @default.
• W2127497500 hasPublicationYear "1997" @default.
• W2127497500 type Work @default.
• W2127497500 sameAs 2127497500 @default.
• W2127497500 citedByCount "14" @default.
• W2127497500 countsByYear W21274975002013 @default.
• W2127497500 countsByYear W21274975002022 @default.
• W2127497500 crossrefType "journal-article" @default.
• W2127497500 hasAuthorship W2127497500A5061902661 @default.
• W2127497500 hasBestOaLocation W21274975001 @default.
• W2127497500 hasConcept C105795698 @default.
• W2127497500 hasConcept C121332964 @default.
• W2127497500 hasConcept C12287442 @default.
• W2127497500 hasConcept C168110828 @default.
• W2127497500 hasConcept C17599544 @default.
• W2127497500 hasConcept C182358072 @default.
• W2127497500 hasConcept C191897082 @default.
• W2127497500 hasConcept C192562407 @default.
• W2127497500 hasConcept C33024259 @default.
• W2127497500 hasConcept C33923547 @default.
• W2127497500 hasConcept C44870925 @default.
• W2127497500 hasConcept C50425793 @default.
• W2127497500 hasConcept C68709404 @default.
• W2127497500 hasConcept C87040749 @default.
• W2127497500 hasConcept C98444146 @default.
• W2127497500 hasConceptScore W2127497500C105795698 @default.
• W2127497500 hasConceptScore W2127497500C121332964 @default.
• W2127497500 hasConceptScore W2127497500C12287442 @default.
• W2127497500 hasConceptScore W2127497500C168110828 @default.
• W2127497500 hasConceptScore W2127497500C17599544 @default.
• W2127497500 hasConceptScore W2127497500C182358072 @default.
• W2127497500 hasConceptScore W2127497500C191897082 @default.
• W2127497500 hasConceptScore W2127497500C192562407 @default.
• W2127497500 hasConceptScore W2127497500C33024259 @default.
• W2127497500 hasConceptScore W2127497500C33923547 @default.
• W2127497500 hasConceptScore W2127497500C44870925 @default.
• W2127497500 hasConceptScore W2127497500C50425793 @default.
• W2127497500 hasConceptScore W2127497500C68709404 @default.
• W2127497500 hasConceptScore W2127497500C87040749 @default.
• W2127497500 hasConceptScore W2127497500C98444146 @default.
• W2127497500 hasIssue "1" @default.
• W2127497500 hasLocation W21274975001 @default.
• W2127497500 hasLocation W21274975002 @default.
• W2127497500 hasOpenAccess W2127497500 @default.
• W2127497500 hasPrimaryLocation W21274975001 @default.
• W2127497500 hasRelatedWork W165935137 @default.
• W2127497500 hasRelatedWork W2012263400 @default.
• W2127497500 hasRelatedWork W2052033957 @default.
• W2127497500 hasRelatedWork W2075449560 @default.
• W2127497500 hasRelatedWork W2116228165 @default.
• W2127497500 hasRelatedWork W2127497500 @default.
• W2127497500 hasRelatedWork W2963789724 @default.
• W2127497500 hasRelatedWork W2995493500 @default.
• W2127497500 hasRelatedWork W3098174363 @default.
• W2127497500 hasRelatedWork W3104236707 @default.
• W2127497500 hasVolume "487" @default.
• W2127497500 isParatext "false" @default.
• W2127497500 isRetracted "false" @default.

• next