Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |
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Page 530
3n Mr - 3 M 2 ra ( nr + 3M ) and W = 2 " – 3M = 2 - 2 Equations ( 11 ) and ( 12 )
can further be inverted to give ( 14 ) po ? ... By virtue of the foregoing equations it
can be shown that the BardeenPress equation implies the Zerilli ( or the Regge ...
3n Mr - 3 M 2 ra ( nr + 3M ) and W = 2 " – 3M = 2 - 2 Equations ( 11 ) and ( 12 )
can further be inverted to give ( 14 ) po ? ... By virtue of the foregoing equations it
can be shown that the BardeenPress equation implies the Zerilli ( or the Regge ...
Page 586
c ) For the region of density below go , the Harrison - Wheeler ( HW ) equation of
state is used . We will see anyhow that the result for the maximum mass is not
very sensitive to the equation of state employed in this region . The contribution of
...
c ) For the region of density below go , the Harrison - Wheeler ( HW ) equation of
state is used . We will see anyhow that the result for the maximum mass is not
very sensitive to the equation of state employed in this region . The contribution of
...
Page 682
The next term in the neutrino equation is a Fokker - Planck type of equation
representing the energy loss of neutrinos by elastic collisions with electrons . The
element V ( Av / v ) 2 is taken as one - half , which is also the mean energy
exchange ...
The next term in the neutrino equation is a Fokker - Planck type of equation
representing the energy loss of neutrinos by elastic collisions with electrons . The
element V ( Av / v ) 2 is taken as one - half , which is also the mean energy
exchange ...
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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
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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
Bibliographic information
| Title | Proceedings of the International School of Physics "Enrico Fermi.", Volume 65 Proceedings of the International School of Physics "Enrico Fermi.", Società italiana di fisica Rivista del nuovo cimento |
| Contributor | Società italiana di fisica |
| Publisher | N. Zanichelli, 1978 |
| Original from | the University of California |
| Digitized | 14 Aug 2008 |
| ISBN | 0720407206, 9780720407204 |
| Export Citation | BiBTeX EndNote RefMan |