Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
From inside the book
Results 1-3 of 87
Page 309
Asymptotic form of the outgoing burst of gravitational radiation emitted by a
particle of mass m radially falling into a Schwarzschild black hole of mass M . The
diagrams are given as a function of the retarded time ( t — * * ) / M . In a ) the
effective ...
Asymptotic form of the outgoing burst of gravitational radiation emitted by a
particle of mass m radially falling into a Schwarzschild black hole of mass M . The
diagrams are given as a function of the retarded time ( t — * * ) / M . In a ) the
effective ...
Page 315
tation in strong fields of the gravitationally induced electromagnetic radiation [ 63
] . The spectra of both the gravitational and the electromagnetic radiation are
given in fig . 14 . A qualitative explanation of this process has been given 0 . 04 0
.
tation in strong fields of the gravitationally induced electromagnetic radiation [ 63
] . The spectra of both the gravitational and the electromagnetic radiation are
given in fig . 14 . A qualitative explanation of this process has been given 0 . 04 0
.
Page 332
The trajectories of the particles along the common direction of the fields E , and B
, as seen in the new Lorentz frame are given by the following expression d . xx (
58 ) = E , EX + B . B « . Here 2 is an appropriately normalized parameter ...
The trajectories of the particles along the common direction of the fields E , and B
, as seen in the new Lorentz frame are given by the following expression d . xx (
58 ) = E , EX + B . B « . Here 2 is an appropriately normalized parameter ...
What people are saying - Write a review
We haven't found any reviews in the usual places.
Contents
Why are the stars as they are? | 1 |
Krzeminskis StarCen | 5 |
The theory of degenerate configurations the limiting | 7 |
Copyright | |
64 other sections not shown
Other editions - View all
Common terms and phrases
absorption accretion amplitude analysis antenna approximation assumed Astrophys BAHCALL binary black hole calculated colors considered consistent core corresponding cycle Cyg X-1 density dependence detail detected detectors determined dips discussed disk distance eclipse effect electromagnetic electron emission energy equation estimate existence expected field Figure flux frequency function geometry give given gravitational gravitational collapse important increases indicated intensity interesting Journ less Lett light curve limit lines magnetic mass measurements motion Nature neutron star noise observed obtained occur optical orbital parameters particle period phase Phys position possible potential present primary pulsations pulse radiation radio range ratio region relative rotation scale sensitivity shown shows spectrum stellar stellar wind suggested surface temperature transducer values variable variations velocity X-ray sources