Einstein’s Geometrical Versus Feynman’s Quantum-Field Approaches to Gravity Physics: Testing by Modern Multimessenger Astronomy

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Einstein’s Geometrical Versus Feynman’s Quantum-Field Approaches to Gravity Physics: Testing by Modern Multimessenger Astronomy. / Baryshev, Yurij .

In: Universe, Vol. 6, No. 11, 212, 18.11.2020.

Research output: Contribution to journal › Article › peer-review

BibTeX

@article{749258031c7746da89902356644f1c9a,

title = "Einstein{\textquoteright}s Geometrical Versus Feynman{\textquoteright}s Quantum-Field Approaches to Gravity Physics: Testing by Modern Multimessenger Astronomy",

abstract = "Modern multimessenger astronomy delivers unique opportunity for performing crucial observations that allow for testing the physics of the gravitational interaction. These tests include detection of gravitational waves by advanced LIGO-Virgo antennas, Event Horizon Telescope observations of central relativistic compact objects (RCO) in active galactic nuclei (AGN), X-ray spectroscopic observations of Fe Ka line in AGN, Galactic X-ray sources measurement of masses and radiuses of neutron stars, quark stars, and other RCO. A very important task of observational cosmology is to perform large surveys of galactic distances independent on cosmological redshifts fortesting the nature of the Hubble law and peculiar velocities. Forthcoming multimessenger astronomy, while using such facilities as advanced LIGO-Virgo, Event Horizon Telescope (EHT), ALMA, WALLABY, JWST, EUCLID, and THESEUS, can elucidate the relation between Einstein{\textquoteright}s geometrical and Feynman{\textquoteright}s quantum-field approaches to gravity physics and deliver a new possibilities forunification of gravitation with other fundamental quantum physical interactions.",

keywords = "gravitation; cosmology; multimessenger astronomy; quantum physics, gravitation; cosmology; multimessenger astronomy; quantum physics",

author = "Yurij Baryshev",

note = "Baryshev, Y. Einstein{\textquoteright}s Geometrical Versus Feynman{\textquoteright}s Quantum-Field Approaches to Gravity Physics: Testing by Modern Multimessenger Astronomy. Universe 2020, 6, 212.",

year = "2020",

month = nov,

day = "18",

language = "English",

volume = "6",

journal = "Universe",

issn = "2218-1997",

publisher = "MDPI AG",

number = "11",

}

RIS

TY - JOUR

T1 - Einstein’s Geometrical Versus Feynman’s Quantum-Field Approaches to Gravity Physics: Testing by Modern Multimessenger Astronomy

AU - Baryshev, Yurij

N1 - Baryshev, Y. Einstein’s Geometrical Versus Feynman’s Quantum-Field Approaches to Gravity Physics: Testing by Modern Multimessenger Astronomy. Universe 2020, 6, 212.

PY - 2020/11/18

Y1 - 2020/11/18

N2 - Modern multimessenger astronomy delivers unique opportunity for performing crucial observations that allow for testing the physics of the gravitational interaction. These tests include detection of gravitational waves by advanced LIGO-Virgo antennas, Event Horizon Telescope observations of central relativistic compact objects (RCO) in active galactic nuclei (AGN), X-ray spectroscopic observations of Fe Ka line in AGN, Galactic X-ray sources measurement of masses and radiuses of neutron stars, quark stars, and other RCO. A very important task of observational cosmology is to perform large surveys of galactic distances independent on cosmological redshifts fortesting the nature of the Hubble law and peculiar velocities. Forthcoming multimessenger astronomy, while using such facilities as advanced LIGO-Virgo, Event Horizon Telescope (EHT), ALMA, WALLABY, JWST, EUCLID, and THESEUS, can elucidate the relation between Einstein’s geometrical and Feynman’s quantum-field approaches to gravity physics and deliver a new possibilities forunification of gravitation with other fundamental quantum physical interactions.

AB - Modern multimessenger astronomy delivers unique opportunity for performing crucial observations that allow for testing the physics of the gravitational interaction. These tests include detection of gravitational waves by advanced LIGO-Virgo antennas, Event Horizon Telescope observations of central relativistic compact objects (RCO) in active galactic nuclei (AGN), X-ray spectroscopic observations of Fe Ka line in AGN, Galactic X-ray sources measurement of masses and radiuses of neutron stars, quark stars, and other RCO. A very important task of observational cosmology is to perform large surveys of galactic distances independent on cosmological redshifts fortesting the nature of the Hubble law and peculiar velocities. Forthcoming multimessenger astronomy, while using such facilities as advanced LIGO-Virgo, Event Horizon Telescope (EHT), ALMA, WALLABY, JWST, EUCLID, and THESEUS, can elucidate the relation between Einstein’s geometrical and Feynman’s quantum-field approaches to gravity physics and deliver a new possibilities forunification of gravitation with other fundamental quantum physical interactions.

KW - gravitation; cosmology; multimessenger astronomy; quantum physics

UR - https://www.mdpi.com/2218-1997/6/11/212

M3 - Article

VL - 6

JO - Universe

JF - Universe

SN - 2218-1997

IS - 11

M1 - 212

ER -

ID: 70953799