Search Results - "Morsink, S"

THE IMPACT OF SURFACE TEMPERATURE INHOMOGENEITIES ON QUIESCENT NEUTRON STAR RADIUS MEASUREMENTS by Elshamouty, K. G., Heinke, C. O., Morsink, S. M., Bogdanov, S., Stevens, A. L.

“…ABSTRACT Fitting the thermal X-ray spectra of neutron stars (NSs) in quiescent X-ray binaries can constrain the masses and radii of NSs. The effect of…”
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NEUTRON STAR MASS-RADIUS CONSTRAINTS USING EVOLUTIONARY OPTIMIZATION by Stevens, A. L., Fiege, J. D., Leahy, D. A., Morsink, S. M.

“…ABSTRACT The equation of state of cold supra-nuclear-density matter, such as in neutron stars, is an open question in astrophysics. A promising method for…”
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Normal Modes of Rotating Magnetic Stars by Morsink, S. M, Rezania, V

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Eye movement desensitization and reprocessing (EMDR) treatment in the medical setting: A systematic review by Driessen, H., Morsink, S., Van Busschbach, J., Kranenburg, L.

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The Effect of Neutron Star Gravitational Binding Energy on Gravitational Radiation-driven Mass-Transfer Binaries by Alécian, Evelyne, Morsink, Sharon M

“…In a relativistic model of a neutron star, the star's mass is less than the mass of the individual component baryons, because the star's negative binding…”
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The Radius of PSR J0740+6620 from NICER and XMM-Newton Data by Miller, M. C, Lamb, F. K, Dittmann, A. J, Bogdanov, S, Arzoumanian, Z, Gendreau, K. C, Guillot, S, Ho, W. C. G, Lattimer, J. M, Loewenstein, M, Morsink, S. M, Ray, P. S, Wolff, M. T, Baker, C. L, Cazeau, T, Manthripragada, S, Markwardt, C. B, Okajima, T, Pollard, S, Cognard, I, Cromartie, H. T, Fonseca, E, Guillemot, L, Kerr, M, Parthasarathy, A, Pennucci, T. T, Ransom, S, Stairs, I

“…PSR J0740$+$6620 has a gravitational mass of $2.08\pm 0.07~M_\odot$, which is the highest reliably determined mass of any neutron star. As a result, a…”
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Semiclassical gravity in 1+1 dimensions by MANN, R. B, MORSINK, S. M, SIKKEMA, A. E, STEELE, T. G

“…Relativistic wave equations are solved exactly in the classical space-time background of a two-dimensional gravitational theory. In the simplest nontrivial…”
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Pulse Shapes from Rapidly Rotating Neutron Stars: Equatorial Photon Orbits by Cadeau, Coire, Leahy, Denis A, Morsink, Sharon M

“…We demonstrate that fitted values of the stellar radius obtained by fitting theoretical light curves to observations of millisecond-period X-ray pulsars can…”
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A NICER view of PSR J0030+0451: Implications for the dense matter equation of state by Raaijmakers, G, Riley, T. E, Watts, A. L, Greif, S. K, Morsink, S. M, Hebeler, K, Schwenk, A, Hinderer, T, Nissanke, S, Guillot, S, Arzoumanian, Z, Bogdanov, S, Gendreau, D. Chakrabarty K. C, Ho, W. C. G, Lattimer, J. M, Ludlam, R. M, Wolff, M. T

“…ApJ Letters, 887, L22 (2019) Both the mass and radius of the millisecond pulsar PSR J0030+0451 have been inferred via pulse-profile modeling of X-ray data…”
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PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter by Miller, M. C, Lamb, F. K, Dittmann, A. J, Bogdanov, S, Arzoumanian, Z, Gendreau, K. C, Guillot, S, Harding, A. K, Ho, W. C. G, Lattimer, J. M, Ludlam, R. M, Mahmoodifar, S, Morsink, S. M, Ray, P. S, Strohmayer, T. E, Wood, K. S, Enoto, T, Foster, R, Okajima, T, Prigozhin, G, Soong, Y

“…ApJL 2019, 887, L24 Neutron stars are not only of astrophysical interest, but are also of great interest to nuclear physicists, because their attributes can be…”
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Neutron Star Mass-Radius Constraints using Evolutionary Optimization by Stevens, A. L, Fiege, J. D, Leahy, D. A, Morsink, S. M

“…The equation of state of cold supra-nuclear-density matter, such as in neutron stars, is an open question in astrophysics. A promising method for constraining…”
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Quasi-normal Modes of Rotating Relativistic Stars: Neutral Modes for Realistic Equations of State by Morsink, Sharon M, Stergioulas, Nikolaos, Blattnig, Steve R

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Light Curves for Rapidly Rotating Neutron Stars by Cadeau, Coire, Morsink, Sharon M, Leahy, Denis, Campbell, Sheldon S

“…We present ray-tracing computations for light emitted from the surface of a rapidly rotating neutron star in order to construct light curves for X-ray pulsars…”
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Limits on Mass and Radius for the Millisecond-Period X-Ray Pulsar SAX J1808.4–3658 by Leahy, Denis A, Morsink, Sharon M, Cadeau, Coire

“…SAX J1808.4-3658 has a 2.5 ms neutron star rotation period and exhibits X-ray pulsations due to its rotating hot spot. Here we present an analysis of the pulse…”
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Saturation of the r-Mode Instability by Arras, Phil, Flanagan, Eanna E, Morsink, Sharon M, Schenk, A. Katrin, Teukolsky, Saul A, Wasserman, Ira

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Rotational Broadening of Atomic Spectral Features from Neutron Stars by Chang, Philip, Morsink, Sharon, Bildsten, Lars, Wasserman, Ira

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ASTROPHYSICS: Signs of Extreme Gravity by Morsink, S

“…Neutron stars are among the densest objects in the universe, and observations of processes in their vicinity may provide insights into conditions of extreme…”
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Signs of Extreme Gravity by Morsink, Sharon

“…Neutron stars are created in the cores of massive stars during supernova explosions. For gravitational physicists, the most exciting aspect of a neutron star…”
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Quantum effects in black hole interiors by ANDERSON, W. G, BRADY, P. R, ISRAEL, W, MORSINK, S. M

“…The Weyl curvature inside a black hole formed in a generic collapse grows, classically without bound, near to the inner horizon, due to partial absorption and…”
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Structure of the charged spherical black hole interior by Bonanno, A., Droz, S., Israel, Werner, Morsink, S. M.

“…The internal structure of a charged spherical black hole is still a topic of debate. In a non-rotating but aspherical gravitational collapse to form a…”
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