Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
High-redshift long gamma-ray bursts Hubble diagram as a test of basic cosmological relations. / Shirokov, Stanislav I. ; Sokolov, Ilia V. ; Lovyagin, Nikita Yu. ; Baryshev, Yurij V. ; Sokolov, V. V.; Gorokhov, V.L.
в: Monthly Notices of the Royal Astronomical Society, Том 496, № 2, 03.06.2020, стр. 1530–1544.Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
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TY - JOUR
T1 - High-redshift long gamma-ray bursts Hubble diagram as a test of basic cosmological relations
AU - Shirokov, Stanislav I.
AU - Sokolov, Ilia V.
AU - Lovyagin, Nikita Yu.
AU - Baryshev, Yurij V.
AU - Sokolov, V. V.
AU - Gorokhov, V.L.
PY - 2020/6/3
Y1 - 2020/6/3
N2 - We examine the prospects of the high-redshift long gamma-ray bursts (LGRBs) Hubble diagram as a test of the basic cosmological principles. Analysis of the Hubble diagram allows us to test several fundamental cosmological principles using the directly observed flux–distance–redshift relation. Modern LGRBs data together with the correlation between the spectral peak energy and the isotropic equivalent radiated energy (the so-called Amati relation) can be used for construction of the Hubble diagram at the model-independent level. We emphasize observational selection effects, which inevitably exist and distort the theoretically predicted relations. An example is the weak and strong gravitational lensing bias effect for high-redshift LGRB in the presence of limited observational sensitivity (Malmquist bias). After bias correction, there is a tendency to vacuum-dominated models with ΩΛ→0.9, Ωm → 0.1. Forthcoming gamma-ray observations by the Transient High-Energy Sky and Early Universe Surveyor (THESEUS) space mission together with ground- and space-based multimessenger facilities will allow us to improve essentially the restrictions on alternative basic principles of cosmological models.
AB - We examine the prospects of the high-redshift long gamma-ray bursts (LGRBs) Hubble diagram as a test of the basic cosmological principles. Analysis of the Hubble diagram allows us to test several fundamental cosmological principles using the directly observed flux–distance–redshift relation. Modern LGRBs data together with the correlation between the spectral peak energy and the isotropic equivalent radiated energy (the so-called Amati relation) can be used for construction of the Hubble diagram at the model-independent level. We emphasize observational selection effects, which inevitably exist and distort the theoretically predicted relations. An example is the weak and strong gravitational lensing bias effect for high-redshift LGRB in the presence of limited observational sensitivity (Malmquist bias). After bias correction, there is a tendency to vacuum-dominated models with ΩΛ→0.9, Ωm → 0.1. Forthcoming gamma-ray observations by the Transient High-Energy Sky and Early Universe Surveyor (THESEUS) space mission together with ground- and space-based multimessenger facilities will allow us to improve essentially the restrictions on alternative basic principles of cosmological models.
KW - cosmological parameters
KW - distance scale
KW - Gamma-Ray Bursts
UR - https://www.researchgate.net/publication/341803339_High-redshift_long_gamma-ray_bursts_Hubble_diagram_as_a_test_of_basic_cosmological_relations
UR - https://academic.oup.com/mnras/article-abstract/496/2/1530/5850785?redirectedFrom=fulltext
M3 - Article
VL - 496
SP - 1530
EP - 1544
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
SN - 0035-8711
IS - 2
ER -
ID: 61797545