Results 181 to 190 of about 4,253 (219)
Enhanced theta oscillations in the left temporoparietal region associated with refractory positive symptoms in schizophrenia. [PDF]
Schizophrenia (Heidelb)Wang X +8 more
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Accreting White Dwarfs: An Unreview. [PDF]
Space Sci RevScaringi S, Knigge C, de Martino D.
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Circuit-level dynamics and propagation of slow wave activity modulate their interplay during the awakening process. [PDF]
iSciencePazienti A +4 more
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Uropathogenic Escherichia coli proliferate as a coccoid morphotype inside human host cells. [PDF]
PLoS BiolPokhrel A +5 more
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Let there be multifunctionality: Uncovering the criticality zoo of the AC-DC genetic circuit
Maretvadakethope S +5 more
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Physical Review Letters, 1991
We study a new type of self-gravitating object, described by a soliton solution to the coupled system of the Einstein equation and a matter field equation. The solution describing the self-gravitating object is not static but, instead, is periodic, with both the spacetime geometry and the matter field oscillating in time.
, Seidel, , Suen
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We study a new type of self-gravitating object, described by a soliton solution to the coupled system of the Einstein equation and a matter field equation. The solution describing the self-gravitating object is not static but, instead, is periodic, with both the spacetime geometry and the matter field oscillating in time.
, Seidel, , Suen
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2000
We study the relativistic quadrupole oscillations (ι= 2) of strange quark stars by calculating their quasi-normal modes, and we thus explore the possibility of using these oscillation frequencies and damping times to differentiate among relativistic polytropic stars, neutron stars, pure light-quark stars, and hybrid neutron stars with quark cores.
C. W. Yip, M. C. Chu, P. T. Leung
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We study the relativistic quadrupole oscillations (ι= 2) of strange quark stars by calculating their quasi-normal modes, and we thus explore the possibility of using these oscillation frequencies and damping times to differentiate among relativistic polytropic stars, neutron stars, pure light-quark stars, and hybrid neutron stars with quark cores.
C. W. Yip, M. C. Chu, P. T. Leung
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Adiabatic Oscillations of Stars
Publications of the Astronomical Society of Australia, 1970In the past a number of analytical solutions have been found to the differential equation for small radial adiabatic oscillations of stars, with the aid of a series expansion of the form leading to a two-term recurrence relation.
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2008
A brief introduction to the rapidly oscillating Ap (roAp) stars and a review of their properties is presented. Evidence which strongly suggests that the roAp stars pulsate obliquely in high-overtone, low-degree modes is shown. This review then concentrates on four problems of particular interest to asteroseismologists: 1) The interpretation of the ...
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A brief introduction to the rapidly oscillating Ap (roAp) stars and a review of their properties is presented. Evidence which strongly suggests that the roAp stars pulsate obliquely in high-overtone, low-degree modes is shown. This review then concentrates on four problems of particular interest to asteroseismologists: 1) The interpretation of the ...
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Oscillation Periods of Neutron Stars
Nature, 1965Effect of three-body nuclear potential and two neutron-neutron potentials on radial oscillation periods of neutron ...
SACHIKO TSURUTA +2 more
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