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

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Page 303

The radial effective potentials are here represented for the

The radial effective potentials are here represented for the

**positive**. and negative - root solutions E = ( r ) of test particles a ) with angular momentum / u M = 2 V5 around a Schwarzschild black hole , and b ) with Olu M = -5 ...Page 320

r = 3M / 2 Elu 1.25 1.00

r = 3M / 2 Elu 1.25 1.00

**positive**- root states of**positive**energy 0.75 region 0.50 F 0.25 ! i negative - root states of**positive**energy 0**positive**- root states of negative -0.25 fenergy -0.50 forbidden -0.75 negative - root states of ...Page 342

The basic step in applying the Klein - Sauter - Heisenberg - Euler approach to black - hole physics came from establishing a direct analogy between the E + and E solutions of a quantum field and the

The basic step in applying the Klein - Sauter - Heisenberg - Euler approach to black - hole physics came from establishing a direct analogy between the E + and E solutions of a quantum field and the

**positive**and negative - root ...### What people are saying - Write a review

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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