The gravitational effect on induced charge density for an obliquely rotating neutron start

F De Paolis; A Qadir; IH Tarman

The gravitational effect on induced charge density for an obliquely rotating neutron start

F De Paolis, A Qadir, IH Tarman

King Fahd University of Petroleum & Minerals

Research output: Contribution to journal › Article › peer-review

Abstract

The effect on the induced charge density of the gravitational field of a rotating neutron star with its magnetic axis inclined with respect to the rotational axis is investigated. While gravitation increases the charge density the obliquity reduces it.

Original language	English
Journal	Il Nuovo Cimento B Series 11
State	Published - 1999

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title = "The gravitational effect on induced charge density for an obliquely rotating neutron start",

abstract = "The effect on the induced charge density of the gravitational field of a rotating neutron star with its magnetic axis inclined with respect to the rotational axis is investigated. While gravitation increases the charge density the obliquity reduces it.",

author = "\{De Paolis\}, F and A Qadir and IH Tarman",

year = "1999",

language = "English",

}

TY - JOUR

T1 - The gravitational effect on induced charge density for an obliquely rotating neutron start

AU - De Paolis, F

AU - Qadir, A

AU - Tarman, IH

PY - 1999

Y1 - 1999

N2 - The effect on the induced charge density of the gravitational field of a rotating neutron star with its magnetic axis inclined with respect to the rotational axis is investigated. While gravitation increases the charge density the obliquity reduces it.

AB - The effect on the induced charge density of the gravitational field of a rotating neutron star with its magnetic axis inclined with respect to the rotational axis is investigated. While gravitation increases the charge density the obliquity reduces it.

M3 - Article

SN - 0369-3554

JO - Il Nuovo Cimento B Series 11

JF - Il Nuovo Cimento B Series 11

ER -

The gravitational effect on induced charge density for an obliquely rotating neutron start

Abstract

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