Constraints on cosmological parameters from gamma-ray burst peak photon energy and bolometric fluence measurements and other data

Abstract

We use measurements of the peak photon energy and bolometric fluence of 119 gamma-ray bursts (GRBs) extending over the redshift range of $0.3399\le z\le 8.2$ to simultaneously determine cosmological and Amati relation parameters in six different cosmological models. The resulting Amati relation parameters are almost identical in all six cosmological models, thus validating the use of the Amati relation in standardizing these GRBs. The GRB data cosmological parameter constraints are consistent with, but significantly less restrictive than, those obtained from a joint analysis of baryon acoustic oscillation and Hubble parameter measurements.

arXiv commentMNRAS accepted version

References in corpus (84)

• emcee: The MCMC Hammer
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
• Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
• Intrinsic spectra and energetics of BeppoSAX Gamma-Ray Bursts with known redshifts
• The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
• Cosmological implications of baryon acoustic oscillation (BAO) measurements
• The collimation--corrected GRB energies correlate with the peak energy of their $\nu F_{\nu }$ spectrum
• Calibration of the Tip of the Red Giant Branch (TRGB)
• Dark Energy Survey Year 1 Results: Constraints on Extended Cosmological Models from Galaxy Clustering and Weak Lensing
• Hubble parameter measurement constraints on the cosmological deceleration-acceleration transition redshift
• Measuring the cosmological parameters with the Ep,i-Eiso correlation of Gamma-Ray Bursts
• Gamma-Ray Bursts as a Probe of the Very High Redshift Universe
• Gamma-Ray Bursts as a Probe of the Very High Redshift Universe
• Hubble parameter measurement constraints on the redshift of the deceleration-acceleration transition, dynamical dark energy, and space curvature
• Hubble Parameter and Baryon Acoustic Oscillation Measurement Constraints on the Hubble Constant, the Deviation from the Spatially-Flat $\Lambda$cdm Model, The Deceleration-Acceleration Transition Redshift, and Spatial Curvature
• Model-Independent Multi-Variable Gamma-Ray Burst Luminosity Indicator and Its Possible Cosmological Implications
• Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data
• $H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method
• Baryon acoustic oscillations at z = 2.34 from the correlations of Ly$\alpha$ absorption in eBOSS DR14
• A Hubble Diagram for Quasars
• Median Statistics, H_0, and the Accelerating Universe
• Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0
• The BAO+BBN take on the Hubble tension
• Baryon Acoustic Oscillations and the Hubble Constant: Past, Present and Future
• A Cosmology-Independent Calibration of Gamma-Ray Burst Luminosity Relations and the Hubble Diagram
• Measuring the Hubble constant with Type Ia supernovae as near-infrared standard candles
• General Cosmography Model with Spatial Curvature
• Possible signals of vacuum dynamics in the Universe
• An improved model-independent assessment of the late-time cosmic expansion
• A blinded determination of $H_0$ from low-redshift Type Ia supernovae, calibrated by Cepheid variables
• Determining the Hubble constant from Hubble parameter measurements
• Addressing the circularity problem in the $E_{\text{p}}-E_{\text{iso}}$ correlation of Gamma-Ray Bursts
• Baryon acoustic oscillation, Hubble parameter, and angular size measurement constraints on the Hubble constant, dark energy dynamics, and spatial curvature
• Ultra-compact structure in intermediate-luminosity radio quasars: building a sample of standard cosmological rulers and improving the dark energy constraints up to $z\sim 3$
• Using the tilted flat-$\Lambda$CDM and the untilted non-flat $\Lambda$CDM inflation models to measure cosmological parameters from a compilation of observational data
• Constraints on dark energy dynamics and spatial curvature from Hubble parameter and baryon acoustic oscillation data
• Cosmology with gamma-ray bursts: II Cosmography challenges and cosmological scenarios for the accelerated Universe
• Using quasar X-ray and UV flux measurements to constrain cosmological model parameters
• Non-Gaussian Error Distribution of Hubble Constant Measurements
• Gamma-Ray Bursts in $1.8<z<5.6$ Suggest that the Time Variation of the Dark Energy is Small
• An independent determination of the local Hubble constant
• Measuring dark energy with the $E_{\mathrm{iso}}-E_{\mathrm{p}}$ correlation of gamma-ray bursts using model-independent methods
• A new measurement of the Hubble constant and matter content of the Universe using extragalactic background light $\gamma$-ray attenuation
• Observational constraints on the tilted spatially-flat and the untilted nonflat $\varphi$CDM dynamical dark energy inflation models
• Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters
• Planck 2015 constraints on the non-flat $\Lambda$CDM inflation model
• Cosmological Constraints from Compact Radio Source Angular Size versus Redshift Data
• Dynamical dark energy: scalar fields and running vacuum
• Binned Hubble parameter measurements and the cosmological deceleration-acceleration transition
• Cosmological Models and Gamma-Ray Bursts Calibrated by Using Pade Method
• Measuring the Hubble constant and spatial curvature from supernova apparent magnitude, baryon acoustic oscillation, and Hubble parameter data
• Constraining cosmic curvature by using age of galaxies and gravitational lenses
• New Model-independent Method to Test the Curvature of the Universe
• Constraints on non-flat cosmologies with massive neutrinos after Planck 2015
• Spectral analysis of Fermi-LAT gamma-ray bursts with known redshift and their potential use as cosmological standard candles
• Using SPTpol, Planck 2015, and non-CMB data to constrain tilted spatially-flat and untilted non-flat $\Lambda$CDM, XCDM, and $\varphi$CDM dark energy inflation cosmologies
• Independent Cosmological Constraints from high-z HII Galaxies
• Nonflat time-variable dark energy cosmology
• Planck 2015 constraints on the non-flat $\varphi$CDM inflation model
• Constraining dark energy with gamma-ray bursts
• Model-independent Curvature Determination from Gravitational-Wave Standard Sirens and Cosmic Chronometers
• An evaluation of cosmological models from expansion and growth of structure measurements
• Towards a Precision Cosmology from Starburst Galaxies at z>2
• Observational constraints on the tilted flat-XCDM and the untilted nonflat XCDM dynamical dark energy inflation parameterizations
• CMB tensions with low-redshift $H_0$ and $S_8$ measurements: impact of a redshift-dependent type-Ia supernovae intrinsic luminosity
• Primordial power spectra for curved inflating universes
• Planck 2015 constraints on the non-flat XCDM inflation model
• Observational constraints on non-flat dynamical dark energy cosmological models
• Planck 2015 constraints on spatially-flat dynamical dark energy models
• Constraints on dark energy from H II starburst galaxy apparent magnitude versus redshift data
• Low redshift observational constraints on tachyon models of dark energy
• Constraints on dark energy from the lookback time versus redshift test
• Galaxy cluster number count data constraints on cosmological parameters
• Standardizing the GRBs with the Amati Ep,i - Eiso relation: the updated Hubble diagram and implications for cosmography
• Model-independent distance calibration of high-redshift gamma-ray bursts and constrain on the $\Lambda$CDM model
• Exploring Parameter Constraints on Quintessential Dark Energy: the Inverse Power Law Model
• Observational constraints on quintessence models of dark energy
• First study of reionization in tilted flat and untilted non-flat dynamical dark energy inflation models
• Using the Extragalactic Gamma-Ray Background to Constrain the Hubble Constant and Matter Density of the Universe
• Effect of the spatial curvature of the Universe on the form of the gravitational potential
• Spatial Curvature in Cosmology Revisited
• Flatness without CMB - the Entanglement of Spatial Curvature and Dark Energy Equation of State
• Measuring $H_0$ from low-$z$ datasets

Cited by in corpus (56)

• Challenges for $\Lambda$CDM: An update
• Eppur è piatto? The cosmic chronometer take on spatial curvature and cosmic concordance
• Non-parametric spatial curvature inference using late-universe cosmological probes
• The galaxy power spectrum take on spatial curvature and cosmic concordance
• Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0{w}_a$CDM cosmological parameterization result
• Using Pantheon and DES supernova, baryon acoustic oscillation, and Hubble parameter data to constrain the Hubble constant, dark energy dynamics, and spatial curvature
• Do gamma-ray burst measurements provide a useful test of cosmological models?
• Optical and X-ray GRB Fundamental Planes as Cosmological Distance Indicators
• Determining the range of validity of quasar X-ray and UV flux measurements for constraining cosmological model parameters
• Evidence of a decreasing trend for the Hubble constant
• Standardizing Platinum Dainotti-correlated gamma-ray bursts, and using them with standardized Amati-correlated gamma-ray bursts to constrain cosmological model parameters
• Standardizing Dainotti-correlated gamma-ray bursts, and using them with standardized Amati-correlated gamma-ray bursts to constrain cosmological model parameters
• Do quasar X-ray and UV flux measurements provide a useful test of cosmological models?
• Measuring cosmological parameters with a luminosity-time correlation of gamma-ray bursts
• $H_0=69.8\pm 1.3$ $\mathrm{km}{\mathrm{s}}^{-1}\mathrm{Mp}{\mathrm{c}}^{-1}$, ${\Omega }_{m0}=0.288\pm 0.017$, and other constraints from lower-redshift, non-CMB, expansion-rate data
• Cosmological constraints from higher-redshift gamma-ray burst, HII starburst galaxy, and quasar (and other) data
• Gamma-ray burst data strongly favor the three-parameter fundamental plane (Dainotti) correlation relation over the two-parameter one
• Calibrating Gamma-Ray Bursts by Using a Gaussian Process with Type Ia Supernovae
• Testing Dark Energy Models with Gamma-Ray Bursts Calibrated from the Observational $H(z)$ Data through a Gaussian Process
• Gamma ray burst constraints on cosmological models from the improved Amati correlation
• $E_{\mathrm{iso}}$-$E_{\mathrm{p}}$ correlation of gamma ray bursts: calibration and cosmological applications
• Standardizing reverberation-measured C IV time-lag quasars, and using them with standardized Mg II quasars to constrain cosmological parameters
• Observational constraints and predictions of the interacting dark sector with field-fluid mapping
• Is the $w_0{w}_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck CMB anisotropy data?
• Cosmological constraints from HII starburst galaxy, quasar angular size, and other measurements
• The improved Amati correlations from Gaussian copula
• Quasar UV/X-ray relation luminosity distances are shorter than reverberation-measured radius-luminosity relation luminosity distances
• Effects of type Ia supernovae absolute magnitude priors on the Hubble constant value
• Current data are consistent with flat spatial hypersurfaces in the $\Lambda$CDM cosmological model but favor more lensing than the model predicts
• Do reverberation-measured H$\beta$ quasars provide a useful test of cosmology?
• Consistency study of high- and low-accreting Mg ii quasars: No significant effect of the Fe ii to Mg ii flux ratio on the radius-luminosity relation dispersion
• Observational Constraints on Dynamical Dark Energy Models
• Properties of High-Redshift GRBs
• Gamma Rays Bursts: A Viable Cosmological Probe?
• Effect of extinction on quasar luminosity distances determined from UV and X-ray flux measurements
• Constraints from Fermi observations of Long Gamma-Ray Bursts on cosmological parameters
• Does the GRB Duration Depend on Redshift?
• Low redshift calibration of the Amati relation using galaxy clusters
• Testing the standardizability of, and deriving cosmological constraints from, a new Amati-correlated gamma-ray burst data compilation
• Effects of heterogeneous data sets and time-lag measurement techniques on cosmological parameter constraints from MgII and CIV reverberation-mapped quasar data
• Constraints on power law cosmology from cosmic chronometer, standard ruler, and standard candle data
• Low- and high-redshift H II starburst galaxies obey different luminosity-velocity dispersion relations
• Constraints on Cosmological Models with Gamma-Ray Bursts in Cosmology-Independent Way
• Unveiling the Universe with Emerging Cosmological Probes
• Model-independent Gamma-Ray Bursts Constraints on Cosmological Models Using Machine Learning
• Gamma-Ray Bursts Calibrated from the Observational $H(z)$ Data in Artificial Neural Network Framework
• Tilted non-spatially-flat inflation
• Standardizing reverberation-measured Mg II time-lag quasars, by using the radius-luminosity relation, and constraining cosmological model parameters
• Testing the consistency of new Amati-correlated gamma-ray burst dataset cosmological constraints with those from better-established cosmological data
• Updated observational constraints on $\varphi$CDM dynamical dark energy cosmological models
• Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
• Gamma-Ray Bursts Calibrated by Using Artificial Neural Networks from the Pantheon+ Sample
• Calibration of luminosity correlations of gamma-ray bursts using quasars
• Intermediate redshift calibration of Gamma-ray Bursts and cosmic constraints in non-flat cosmology
• A test of Amati relation using HII galaxy distances
• Redshift Evolution of the HII Galaxy $L$-$\sigma$ Relation: Gaussian Process Analysis and Cosmological Implications