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相关论文: Sources of radiation from neutron stars

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Rapidly rotating neutron stars are promising sources of continuous gravitational wave radiation for the LIGO and Virgo interferometers. The majority of neutron stars in our galaxy have not been identified with electromagnetic observations.…

We are still far from understanding how pulsars pulse, how neutron stars are born, what neutron stars can emit, and in which way they do this. In this short communication, I list 18 alternatives -- several of them old, a few of them new --…

天体物理学 · 物理学 2007-05-23 W. Kundt

We study the possibility to detect the gravitational wave background generated by all the neutron stars in the Galaxy with only one gravitational wave interferometric detector. The proposed strategy consists in squaring the detector's…

天体物理学 · 物理学 2014-10-13 A. Giazotto , S. Bonazzola , E. Gourgoulhon

We present a Markov chain Monte Carlo technique for detecting gravitational radiation from a neutron star in laser interferometer data. The algorithm can estimate up to six unknown parameters of the target, including the rotation frequency…

广义相对论与量子宇宙学 · 物理学 2014-11-17 Richard Umstätter , Renate Meyer , Réjean J. Dupuis , John Veitch , Graham Woan , Nelson Christensen

Neutron stars are identified as pulsars, X-ray binary components, central objects of supernovae remnants, or isolated thermally emitting sources, and at distances beyond 120 pc. A population extrapolation suggests 10$^3$ objects within that…

高能天体物理现象 · 物理学 2023-08-09 Gabriel Bihain

In the next few years, the first detections of gravity-wave signals using Earth-based interferometric detectors will begin to provide precious new information about the structure and dynamics of compact bodies such as neutron stars. The…

广义相对论与量子宇宙学 · 物理学 2017-08-23 Michele Vallisneri

The gravitational waves emitted by neutron stars carry unique information about their structure and composition. Direct detection of these gravitational waves, however, is a formidable technical challenge. In a recent study we quantified…

太阳与恒星天体物理 · 物理学 2009-11-13 Anna L. Watts , Badri Krishnan

Gravitational Wave Astronomy is becoming a reality as Earth-based interferometric gravitational-wave detectors reach the design sensitivities and move towards advanced configurations that may lead to gravitational-wave detections in the…

天体物理学 · 物理学 2008-08-05 Carlos F. Sopuerta

Neutron stars are some of the densest manifestations of massive objects in the universe. They are ideal astrophysical laboratories for testing theories of dense matter physics and provide connections among nuclear physics, particle physics…

天体物理学 · 物理学 2011-05-05 J. M. Lattimer , M. Prakash

We discuss different ways that neutron stars can generate gravitational waves, describe recent improvements in modelling the relevant scenarios in the context of improving detector sensitivity, and show how observations are beginning to…

太阳与恒星天体物理 · 物理学 2011-01-28 N. Andersson , V. Ferrari , D. I. Jones , K. D. Kokkotas , B. Krishnan , J. Read , L. Rezzolla , B. Zink

A new generation of observatories is looking for gravitational waves. These waves, emitted by highly relativistic systems, will open a new window for ob- servation of the cosmos when they are detected. Among the most promising sources of…

广义相对论与量子宇宙学 · 物理学 2015-11-11 Warren G. Anderson , Jolien D. E. Creighton

Searches for continuous gravitational waves from \textit{unknown} Galactic neutron stars provide limits on the shapes of neutron stars. A rotating neutron star will produce gravitational waves if asymmetric deformations exist in its…

高能天体物理现象 · 物理学 2021-11-09 Brendan T. Reed , Alex Deibel , C. J. Horowitz

Rapidly spinning neutron stars with non-axisymmetric mass distributions are expected to generate quasi-monochromatic continuous gravitational waves. While many searches for unknown, isolated spinning neutron stars have been carried out,…

广义相对论与量子宇宙学 · 物理学 2015-05-27 E. Goetz , K. Riles

Precise and reliable measurements of the masses and radii of neutron stars with a variety of masses would provide valuable guidance for improving models of the properties of cold matter with densities above the saturation density of nuclear…

高能天体物理现象 · 物理学 2016-04-20 M. Coleman Miller , Frederick K. Lamb

Neutron stars involve extreme physics which is difficult (perhaps impossible) to explore in laboratory experiments. We have to turn to astrophysical observations, and try to extract information from the entire range of the electromagnetic…

高能天体物理现象 · 物理学 2017-09-22 N. Andersson

The X-ray emission of neutron stars enables a probe of their temperatures, geometries, and magnetospheric properties. The current number of X-ray emitting pulsars is insufficient to rule out observational biases that may arise from poorly…

高能天体物理现象 · 物理学 2022-02-09 Armin Vahdat , Bettina Posselt , Andrea Santangelo , George G. Pavlov

Neutron stars are highly compact astrophysical objects and therefore of utmost relevance to learn about theories of gravity. Whereas the proper equation of state of the nuclear matter inside neutron stars is not yet known, and a wide range…

广义相对论与量子宇宙学 · 物理学 2022-04-28 Jutta Kunz

Neutron stars have long been regarded as extra-terrestrial laboratories from which we can learn about extreme energy density matter at low temperatures. In this article, I highlight some of the recent advances made in astrophysical…

太阳与恒星天体物理 · 物理学 2023-07-19 Madappa Prakash

Neutron stars are compact and dense celestial objects that offer the unique opportunity to explore matter and its interactions under conditions that cannot be reproduced elsewhere in the Universe. Their extreme gravitational, rotational and…

高能天体物理现象 · 物理学 2024-01-29 Stefano Ascenzi , Vanessa Graber , Nanda Rea

Neutron stars are excellent emitters of gravitational waves. Squeezing matter beyond nuclear densities invites exotic physical processes, many of which violently transfer large amounts of mass at relativistic velocities, disrupting…

高能天体物理现象 · 物理学 2015-11-20 Paul D. Lasky
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