Excitation of wakefield around pulsars

Vazha I. Berezhiani; Zaza Osmanov; Milivoj Belic

Excitation of wakefield around pulsars

Vazha I. Berezhiani
, Zaza Osmanov^*
, Milivoj Belic

^*Corresponding author for this work

Research output: Contribution to journal › Conference article › peer-review

Abstract

We study the generation of the wakefields by means of the high energy radiation of pulsars. The problem is considered in the framework of a one dimensional approach. We linearize the set of governing equations consisting of the momentum equation, continuity equation and Poisson equation and show that a wavelike structure will inevitably arise relatively close to the pulsar.

Original language	English
Journal	Proceedings of Science
Publication status	Published - 2015
Externally published	Yes
Event	3rd Modern Physics of Compact Stars, MPCS 2015 - Yerevan, Armenia Duration: 30 Sept 2015 → 3 Oct 2015

Cite this

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title = "Excitation of wakefield around pulsars",

abstract = "We study the generation of the wakefields by means of the high energy radiation of pulsars. The problem is considered in the framework of a one dimensional approach. We linearize the set of governing equations consisting of the momentum equation, continuity equation and Poisson equation and show that a wavelike structure will inevitably arise relatively close to the pulsar.",

author = "Berezhiani, \{Vazha I.\} and Zaza Osmanov and Milivoj Belic",

note = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s).; 3rd Modern Physics of Compact Stars, MPCS 2015 ; Conference date: 30-09-2015 Through 03-10-2015",

year = "2015",

language = "English",

journal = "Proceedings of Science",

issn = "1824-8039",

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TY - JOUR

T1 - Excitation of wakefield around pulsars

AU - Berezhiani, Vazha I.

AU - Osmanov, Zaza

AU - Belic, Milivoj

N1 - Publisher Copyright: © Copyright owned by the author(s).

PY - 2015

Y1 - 2015

N2 - We study the generation of the wakefields by means of the high energy radiation of pulsars. The problem is considered in the framework of a one dimensional approach. We linearize the set of governing equations consisting of the momentum equation, continuity equation and Poisson equation and show that a wavelike structure will inevitably arise relatively close to the pulsar.

AB - We study the generation of the wakefields by means of the high energy radiation of pulsars. The problem is considered in the framework of a one dimensional approach. We linearize the set of governing equations consisting of the momentum equation, continuity equation and Poisson equation and show that a wavelike structure will inevitably arise relatively close to the pulsar.

UR - https://www.scopus.com/pages/publications/85053484816

M3 - Conference article

AN - SCOPUS:85053484816

SN - 1824-8039

JO - Proceedings of Science

JF - Proceedings of Science

T2 - 3rd Modern Physics of Compact Stars, MPCS 2015

Y2 - 30 September 2015 through 3 October 2015

ER -

Excitation of wakefield around pulsars

Abstract

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