## Proceedings of the International School of Physics "Enrico Fermi.", Volume 65N. Zanichelli, 1978 - Nuclear physics |

### From inside the book

Results 1-3 of 78

Page 530

2

_ _ - ( W + + 210 ) A _ Y K 2 + = 36 — 2M ... By virtue of the foregoing

can be shown that the BardeenPress

2

**Equations**( 11 ) and ( 12 ) can further be inverted to give ( 14 ) ra ( nr + 3M ) y __ _ - ( W + + 210 ) A _ Y K 2 + = 36 — 2M ... By virtue of the foregoing

**equations**itcan 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 )

state is used . We will see anyhow that the result for the maximum mass is not

very sensitive to the

...

c ) For the region of density below go , the Harrison - Wheeler ( HW )

**equation**ofstate 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

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

Gruppo fotografico del partecipanti al Corso | 1 |

Introduction | 17 |

Сen | 37 |

Copyright | |

61 other sections not shown

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### Common terms and phrases

accretion amplitude angular antenna approximation assumed Astrophys binary black hole calculations condition considered cooling core corresponding density depends detailed detectors determined dips discussed disk distance eclipse effect electron emission energy equation estimate existence expected field flux frequency function given gives gravitational heating important increase indicated intensity interesting Journ less Lett light curve limit lines luminosity magnetic field mass matter mean measured momentum motion Nature neutrino neutron star object observed obtained occur optical orbital parameters particle period phase photons Phys physical plasma possible potential present pressure problem pulsations radiation radio radius range region relation relative rotating scale sensitivity shown shows solution spectrum stellar stellar wind suggested surface temperature values variable variations velocity X-ray source