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

### From inside the book

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Page 79

There are no very simple

enough to measure easily with current techniques . There are three other

observable

connection with ...

There are no very simple

**effects**predicted by this model that appear largeenough to measure easily with current techniques . There are three other

observable

**effects**that have been discussed with varying degrees of care inconnection with ...

Page 429

Thus the

the degeneracy

replaced by Cr - 1 and C , by – C . in eq . ( 36 ) then the cross - section for the ...

Thus the

**effect**of neutral currents on these cross - sections is small compared tothe degeneracy

**effects**mentioned above but is included for consistency . If C , isreplaced by Cr - 1 and C , by – C . in eq . ( 36 ) then the cross - section for the ...

Page 802

Relativistic

where r ; = 6GM | ca ( unless we receive detectable ... For a Kerr metric , however

, there are some

Relativistic

**effects**are unimportant for disks around Schwarzschild black holeswhere r ; = 6GM | ca ( unless we receive detectable ... For a Kerr metric , however

, there are some

**effects**which have potentially observable consequences .### What people are saying - Write a review

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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