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

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Page 438

4 , we write down our general results ( including quadrupole moment as well as

systems . In particular , we carry out a detailed analysis of the pulsar PSR 1913 +

...

4 , we write down our general results ( including quadrupole moment as well as

**spin**effects ) in terms of measurable quantities , for ready application to binarysystems . In particular , we carry out a detailed analysis of the pulsar PSR 1913 +

...

Page 442

Heuristic classical derivation of the

interaction of two arbitrary masses . The motion of a

gravitational field of a large mass , was analyzed in detail by PAPAPETROU [ 7 ,

8 ] ...

Heuristic classical derivation of the

**spin**- dependent terms in the gravitationalinteraction of two arbitrary masses . The motion of a

**spinning**test mass , in thegravitational field of a large mass , was analyzed in detail by PAPAPETROU [ 7 ,

8 ] ...

Page 564

On the «

are valid in the limit h→0 . Recently , BARKER and O ' CONNELL have

calculated the microscopic potential between particles with

On the «

**spin**- orbit interaction » . It must be noted that the preceding discussionsare valid in the limit h→0 . Recently , BARKER and O ' CONNELL have

calculated the microscopic potential between particles with

**spin**, and derived a**spin**...### 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