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相关论文: Frame dragging in black hole-pulsar binaries

200 篇论文

For radio pulsars in orbit with a compact companion, pulsar timing observations have proved to be a powerful tool for identifying the physical nature of the companion. Unfortunately, perhaps the most intriguing system where such a tool…

天体物理学 · 物理学 2009-10-31 N. Wex , S. Kopeikin

We present a study of the gravitational time delay of arrival of signals from binary pulsar systems with rotating black hole companions. In particular, we investigate the strength of this effect (Shapiro delay) as a function of the…

天体物理学 · 物理学 2009-10-30 Pablo Laguna , Alex Wolszczan

We study the effect of light-bending on the signal of a pulsar in binaries with rotating black hole companions, focusing on stellar mass black holes. We show that the impacts of various parameters on the bending delays visually match with…

广义相对论与量子宇宙学 · 物理学 2025-06-09 Jyotijwal Debnath , Manjari Bagchi

Objects orbiting in the presence of a rotating massive body experience a gravitomagnetic frame-dragging effect, known as the Lense-Thirring effect, that has been experimentally confirmed in the weak-field limit. In the strong-field limit,…

广义相对论与量子宇宙学 · 物理学 2022-12-14 Angelo Ricarte , Daniel C. M. Palumbo , Ramesh Narayan , Freek Roelofs , Razieh Emami

Timing a pulsar in a close orbit around the supermassive black hole SgrA* at the center of the Milky Way would open the window for an accurate determination of the black hole parameters and for new tests of General Relativity and…

广义相对论与量子宇宙学 · 物理学 2022-12-06 Bilel Ben-Salem , Eva Hackmann

The deflection of light's trajectory has been studied in many different spacetime geometries in weak and strong gravity, including the special cases of spherically symmetric static and spinning black holes. It is also well known that the…

广义相对论与量子宇宙学 · 物理学 2018-08-22 S. V. Iyer

Dark matter around black holes can induce drag forces through dynamical friction and accretion, potentially affecting the orbital evolution and gravitational wave emission of binary systems. While dynamical friction from scalar field dark…

广义相对论与量子宇宙学 · 物理学 2025-07-29 Shuo Xin , Elias R. Most

We discuss the role of general relativity frame dragging acting on magnetic field lines near a rotating (Kerr) black hole. Near ergosphere the magnetic structure becomes strongly influenced and magnetic null points can develop. We consider…

高能天体物理现象 · 物理学 2015-06-04 V. Karas , O. Kopacek , D. Kunneriath

We propose a new procedure for measuring the spin of a black hole with an unprecedented accuracy based on the gravitational lensing of millisecond pulsars. We derive the basic equations for lensing by a rotating black hole. We show that the…

广义相对论与量子宇宙学 · 物理学 2025-08-28 Amjad Ashoorioon , Mohammad Bagher Jahani Poshteh , Robert B. Mann

We propose a novel method to test the binary black hole (BBH) nature of compact binaries detectable by gravitational wave (GW) interferometers and hence constrain the parameter space of other exotic compact objects. The spirit of the test…

广义相对论与量子宇宙学 · 物理学 2017-09-13 N. V. Krishnendu , K. G. Arun , Chandra Kant Mishra

The classical Penrose process and the collisional Penrose processes involve particles decaying or interacting very close to a spinning black hole, in which some particles acquire negative energy and fall into the black hole while others…

高能天体物理现象 · 物理学 2026-04-08 Shravan Vengalil Menon , Kun Hu , Henric Krawczynski

Radio pulsars in short-period eccentric binary orbits can be used to study both gravitational dynamics and binary evolution. The binary system containing PSR J1141$-$6545 includes a massive white dwarf (WD) companion that formed before the…

We describe early success in the evolution of binary black hole spacetimes with a numerical code based on a generalization of harmonic coordinates. Indications are that with sufficient resolution this scheme is capable of evolving binary…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Frans Pretorius

In a recent letter [N. V. Krishnendu et al., PRL 119, 091101 (2017)] we explored the possibility of probing the binary black hole nature of coalescing compact binaries, by measuring their spin-induced multipole moments, observed in advanced…

广义相对论与量子宇宙学 · 物理学 2019-03-13 N. V. Krishnendu , Chandra Kant Mishra , K. G. Arun

We present an analytic study of the mode-coupling phenomena for a scalar field propagating on a rotating Kerr background. Physically, this phenomena is caused by the dragging of reference frames, due to the black-hole (or star's) rotation.…

广义相对论与量子宇宙学 · 物理学 2010-11-19 Shahar Hod

The values of the bending delays in the signal of a radio pulsar in a binary with a stellar mass black hole as a companion have been calculated accurately within a full general relativistic framework considering the Schwarzchid spacetime…

广义相对论与量子宇宙学 · 物理学 2023-07-26 Jyotijwal Debnath , Manjari Bagchi , Avishek Basu

We comment on a recent study reporting evidence for the general relativistic Lense-Thirring secular precession of the inclination $I$ of the orbital plane to the plane of the sky of the tight binary system PSR J1141-6545 made of a white…

广义相对论与量子宇宙学 · 物理学 2020-06-03 Lorenzo Iorio

Frame dragging (Lense-Thirring effect) is generally associated with rotating astrophysical objects. However, it can also be generated by electromagnetic fields if electric and magnetic fields are simultaneously present. In most models of…

广义相对论与量子宇宙学 · 物理学 2015-07-28 Andrés F. Gutiérrez Ruiz , Leonardo A. Pachón

We propose to use pulsar-black hole binaries as a probe of gravitational collider physics. Induced by the gravitation of the pulsar, the atomic transitions of the boson cloud around the black hole back-react on the orbital motion. This…

高能天体物理现象 · 物理学 2021-02-24 Qianhang Ding , Xi Tong , Yi Wang

All multipole moments of a Kerr black hole are uniquely determined by its mass and spin. Gravitational wave observations can test this prediction by measuring spin-induced multipole moments imprinted on the inspiral phase of compact binary…

广义相对论与量子宇宙学 · 物理学 2026-04-14 Rimo Das , N. V. Krishnendu , M. Saleem , Chandra Kant Mishra , K. G. Arun
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