Results 131 to 140 of about 4,836 (143)

A hot-Jupiter progenitor on a super-eccentric retrograde orbit. [PDF]

Nature
Gupta AF, Millholland SC, Im H, Dong J, Jackson JM, Carleo I, Libby-Roberts J, Delamer M, Giovinazzi MR, Lin ASJ, Kanodia S, Wang XY, Stassun K, Masseron T, Dragomir D, Mahadevan S, Wright J, Alvarado-Montes JA, Bender C, Blake CH, Caldwell D, Cañas CI, Cochran WD, Dalba P, Everett ME, Fernandez P, Golub E, Guillet B, Halverson S, Hebb L, Higuera J, Huang CX, Klusmeyer J, Knight R, Leroux L, Logsdon SE, Loose M, McElwain MW, Monson A, Ninan JP, Nowak G, Palle E, Patel Y, Pepper J, Primm M, Rajagopal J, Robertson P, Roy A, Schneider DP, Schwab C, Schweiker H, Sgro L, Shimizu M, Simard G, Stefánsson G, Stevens DJ, Villanueva S, Wisniewski J, Will S, Ziegler C.   +59 more
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Solving non-Hermitian physics for optical manipulation on a quantum computer. [PDF]

Light Sci Appl
Fan YA, Li X, Wei S, Li Y, Long X, Liu H, Nie X, Ng J, Lu D.   +8 more
europepmc   +1 more source

Editorial: Rising stars in motor neuroscience 2023. [PDF]

Front Hum Neurosci
Carozzo S, Demeco A.
europepmc   +1 more source

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Oscillating soliton stars

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.
Edward Seidel, Wai Mo Suen
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Oscillations of Quark Stars

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, Ming Chung Chu, P. T. Leung
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Oscillations in roAp stars

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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Anharmonic Oscillations of Massive Stars [PDF]

Publications of the Astronomical Society of Australia, 1968
The equation of motion, derived from the basic Lagrangian equations for the conservation of momentum and the conservation of energy, for non-linear non-adiabatic radial oscillations of a pulsating star takes the form
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On the non-radial oscillations of a star

Proceedings of the Royal Society of London. Series A: Mathematical and Physical Sciences, 1991
A complete theory of the non-radial oscillations of a static spherically symmetric distribution of matter, described in terms of an energy density and an isotropic pressure, is developed, ab initio , on the premise that the oscillations are excited by incident gravitational waves.
Subrahmanyan Chandrasekhar, Valeria Ferrari   +1 more
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Non-radial oscillations of a star

Astrophysics and Space Science, 1990
The non-radial oscillations of the homogeneous model of a star have been investigated taking into account the variation of the ratio of the specific heats. The stability of the oscillations thus set in is established.
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Oscillation Periods of Neutron Stars

Nature, 1965
Effect of three-body nuclear potential and two neutron-neutron potentials on radial oscillation periods of neutron ...
A. G. W. Cameron, James P. Wright, Sachiko Tsuruta   +2 more
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