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E u r o S c i C o n J o i n t E v e n t o n
Laser Optics & Photonics and
Atomic & Plasma Science
American Journal of Computer Science and Information Technology
ISSN: 2349-3917
J u l y 1 6 - 1 7 , 2 0 1 8
P r a g u e , C z e c h R e p u b l i c
Page 19
Laser Optics & Photonics and Atomic & Plasma Science 2018
B
y choosing the metric in general relativity as the exact solution to the Einstein
equation that is the time delay data, one can determine the gravitational
redshift on the surface of neutron stars. The author presents the physical metric
that is observed time delay data and using the Kerr metric, the author has shown
the effect of a pulsar’ rotation on gravitational redshift in the determination of
gravitational wave frequency is within 1%. Based on this result, the author has
identified potential pulsar candidates with gravitational wave spectra that will be
critical in the study of gravitational redshift and the relationship between rotation
and gravitational waves of a neutron star.
Biography
YukioTomozawa obtained his DSc in 1961 fromTokyo Universi-
ty. He was an Assistant at Tokyo University (1956) and at Tokyo
University of Education (1957-1959) - Member at the Institute
for Advanced Study, Princeton, NJ (1964-1966). He was an As-
sistant Professor, Associate Professor, Professor and Emeritus
Professor at the University of Michigan, USA. He found that the
Schwarzschild metric does not fit the data of time delay ex-
periment in the field of general relativity. He has introduced a
physical metric which fits the data. It was constructed with the
constraint that the speed of light on the spherical direction is
unchanged from that in vacuum. Thismodification changes the
way we understand the nature of gravity drastically. In particular,
the nature of compact objects, neutron stars and black holes, is
very different from that described by the Schwarzschild metric.
It also explains the dark energy, supernova explosion and high
energy cosmic ray emission from AGN (active galactic nuclei),
massive black hole.
tomozawa@umich.eduPulsar identification of background spectra
of LIGO data
Yukio Tomozawa
University of Michigan, USA
Yukio Tomozawa, Am J Compt Sci Inform Technol 2018, Volume 6
DOI: 10.21767/2349-3917-C1-001