A crucial test of the phantom closed cosmological model

Standard

A crucial test of the phantom closed cosmological model. / Shirokov, S. I. ; Baryshev, Yu. V. .

In: Monthly Notices of the Royal Astronomical Society: Letters, Vol. 499, No. 1, 01.11.2020, p. L101-L104.

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Author

Shirokov, S. I. ; Baryshev, Yu. V. . / A crucial test of the phantom closed cosmological model. In: Monthly Notices of the Royal Astronomical Society: Letters. 2020 ; Vol. 499, No. 1. pp. L101-L104.

BibTeX

@article{12b0c83b00994939bdca25fa17623925,

title = "A crucial test of the phantom closed cosmological model",

abstract = "We suggest a crucial direct-observational test for measuring distinction between the standard ΛCDM model and recently proposed phantom dark energy positive curvature cosmological model. The test is based on the fundamental distance–flux–redshift relation for general Friedmann models. It does not depend on the CMBR data, on the large-scale structure growth models, and also on the value of the Hubble constant H0. Our crucial test can be performed by future gamma-ray burst observations with THESEUS space mission and by using gravitational-wave standard siren observations with modern advanced LIGO–Virgo and also forthcoming LISA detectors.",

keywords = "космология, модели-классификация., cosmological parameters, gamma-ray bursts, Gravitational Waves, gravitational waves, HUBBLE DIAGRAM",

author = "Shirokov, {S. I.} and Baryshev, {Yu. V.}",

year = "2020",

month = nov,

day = "1",

doi = "10.1093/mnrasl/slaa167",

language = "English",

volume = "499",

pages = "L101--L104",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Wiley-Blackwell",

number = "1",

}

RIS

TY - JOUR

T1 - A crucial test of the phantom closed cosmological model

AU - Shirokov, S. I.

AU - Baryshev, Yu. V.

PY - 2020/11/1

Y1 - 2020/11/1

N2 - We suggest a crucial direct-observational test for measuring distinction between the standard ΛCDM model and recently proposed phantom dark energy positive curvature cosmological model. The test is based on the fundamental distance–flux–redshift relation for general Friedmann models. It does not depend on the CMBR data, on the large-scale structure growth models, and also on the value of the Hubble constant H0. Our crucial test can be performed by future gamma-ray burst observations with THESEUS space mission and by using gravitational-wave standard siren observations with modern advanced LIGO–Virgo and also forthcoming LISA detectors.

AB - We suggest a crucial direct-observational test for measuring distinction between the standard ΛCDM model and recently proposed phantom dark energy positive curvature cosmological model. The test is based on the fundamental distance–flux–redshift relation for general Friedmann models. It does not depend on the CMBR data, on the large-scale structure growth models, and also on the value of the Hubble constant H0. Our crucial test can be performed by future gamma-ray burst observations with THESEUS space mission and by using gravitational-wave standard siren observations with modern advanced LIGO–Virgo and also forthcoming LISA detectors.

KW - космология

KW - модели-классификация.

KW - cosmological parameters

KW - gamma-ray bursts

KW - Gravitational Waves

KW - gravitational waves

KW - HUBBLE DIAGRAM

UR - https://academic.oup.com/mnrasl/article-abstract/499/1/L101/5911127?redirectedFrom=fulltext

UR - http://www.scopus.com/inward/record.url?scp=85096912408&partnerID=8YFLogxK

UR - https://www.mendeley.com/catalogue/bec39671-9922-3030-8e3d-5f1d67055db8/

U2 - 10.1093/mnrasl/slaa167

DO - 10.1093/mnrasl/slaa167

M3 - Article

VL - 499

SP - L101-L104

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 1

ER -

ID: 69993462