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자연과학대학
물리학전공
Journal papers
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Pulsating neutron star as a source of quasistatic waves of gravity in interstellar medium
Title
Pulsating neutron star as a source of quasistatic waves of gravity in interstellar medium
Authors
Bastrukov S.
;
Molodtsova I.
;
Yang J.
;
Papoyan V.
Ewha Authors
양종만
SCOPUS Author ID
양종만
Issue Date
2005
Journal Title
International Journal of Modern Physics A
ISSN
0217-751X
Citation
International Journal of Modern Physics A vol. 20, no. 32, pp. 7593 - 7602
Indexed
SCI; SCIE; SCOPUS
Document Type
Article
Abstract
The hydrodynamic waves of gravity in the galactic interstellar medium generated by a pulsating neutron star are discussed in this paper. It is shown that the frequency of oscillations of interstellar gas-dust matter in this wave is proportional to that for the g-mode in the neutron star bulk. The corresponding periods are of the millisecond duration. The collective oscillations of charged species in the interstellar wave of gravity can produce electromagnetic radiation, and that the only radio waves of this radiation can freely travel through the galactic gas-dust clouds, suggests that this kind of interstellar waves can manifest itself in the radio range of spectra of a neutron star undergoing pulsations triggered by starquake. This inference is in line with the statement that quasiperiodic micropulses with a time scale of a few milliseconds located in the windows of the main pulse train of the radio pulsar spectra owe their origin to pulsations of neutron stars. © World Scientific Publishing Company.
DOI
10.1142/S0217751X05025425
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