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We study the effect of external companion on the orbital and spin evolution of merging black-hole (BH) binaries. An sufficiently close by and inclined companion can excite Lidov-Kozai (LK) eccentricity oscillations in the binary, thereby…

High Energy Astrophysical Phenomena · Physics 2017-09-05 Bin Liu , Dong Lai

The rotating regular Hayward's spacetime, apart from mass ($M$) and angular momentum ($a$), has an additional deviation parameter ($g$) due to the magnetic charge, which generalizes the Kerr black hole when $g\neq0$, and for $g=0$, it goes…

General Relativity and Quantum Cosmology · Physics 2016-11-03 Muhammed Amir , Fazlay Ahmed , Sushant G. Ghosh

We describe recent numerical simulations of the merger of a class of equal mass, non-spinning, eccentric binary black hole systems in general relativity. We show that with appropriate fine-tuning of the initial conditions to a region of…

General Relativity and Quantum Cosmology · Physics 2008-11-26 Frans Pretorius , Deepak Khurana

Oscillations of photons into axion-like particles in a high-intensity laser field are investigated. Nonlinear QED effects are considered through the low energy behavior of the vacuum polarization tensor, which is derived from the…

High Energy Physics - Phenomenology · Physics 2014-03-03 Selym Villalba-Chávez

The annihilation of pairs of very weakly interacting particles in the neibourghood of gamma-ray sources is introduced here as a plausible mechanism to overcome the baryon load problem. This way we can explain how these very high energy…

Astrophysics · Physics 2011-05-24 Durmus A. Demir , Herman J. Mosquera Cuesta

The Sauter-Schwinger process of electron-positron pair creation from vacuum, driven by a sequence of time-dependent electric-field pulses, is studied in the framework of quantum-field theoretical approach. As demonstrated by our numerical…

High Energy Physics - Phenomenology · Physics 2018-09-19 J. Z. Kamiński , M. Twardy , K. Krajewska

Relativistic electron-positron plasmas are ubiquitous in extreme astrophysical environments such as black holes and neutron star magnetospheres, where accretion-powered jets and pulsar winds are expected to be enriched with such pair…

Light propagating through a perturbed spacetime could imprint the underlying gravitational waveform directly onto electromagnetic observables. In this Letter, we develop a covariant perturbative framework for polarized photon propagation in…

High Energy Astrophysical Phenomena · Physics 2026-05-13 Jiewei Huang , Yehui Hou , Zhen Zhong , Minyong Guo , Bin Chen

Pair-instability should prevent the direct formation of black holes above about $50M_\odot$ creating a pair-instability mass gap. Yet gravitational-wave observations have detected black holes in this mass range. These systems can be…

We investigate electron-positron pair creation from the vacuum in a pulsed electric background field. Employing the Sauter-type pulsed field $E(t)=E_0 {\rm sech}^2 (t/\tau)$ with height $E_0$ and width $\tau$, we demonstrate explicitly the…

High Energy Physics - Phenomenology · Physics 2014-07-30 Hidetoshi Taya , Hirotsugu Fujii , Kazunori Itakura

If at least one neutron star (NS) is magnetized in a binary NS merger, then the orbital motion of the conducting companion during the final inspiral induces a strong voltage and current along the magnetic field lines connecting the NSs. If…

High Energy Astrophysical Phenomena · Physics 2016-08-17 Brian D. Metzger , Charles Zivancev

Black hole (BH) mergers are natural sources of gravitational waves (GWs) and are possibly associated with electromagnetic events. Such events from a charged rotating BH with an accretion on to it could be more energetic and…

High Energy Astrophysical Phenomena · Physics 2024-11-27 Shad Ali

Gamma-ray bursts (GRB) are the most powerful transient phenomena in the Universe. Nowadays dozens of speculations on the origin of GRB were undertaken, but so far a single model for the origin of, in particular, short GRBs does not exist.…

Astrophysics · Physics 2008-07-25 B. E. Zhilyaev , D. L. Dubinovska

We study the dynamical signatures of black hole (BH) and neutron star (NS) binary mergers via Lidov-Kozai oscillations induced by tertiary companions in hierarchical triple systems. For each type of binaries (BH-BH and BH-NS), we explore a…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Bin Liu , Dong Lai , Yi-Han Wang

We propose magnetically arrested disks (MADs) in quiescent black-hole (BH) binaries as the origin of the multiwavelength emission, and argue that this class of sources can dominate the cosmic-ray spectrum around the knee. X-ray luminosities…

High Energy Astrophysical Phenomena · Physics 2021-11-23 Shigeo S. Kimura , Takahiro Sudoh , Kazumi Kashiyama , Norita Kawanaka

We performed ab-initio Particle-In-Cell (PIC) simulations of a pulsar magnetosphere with electron-positron plasma produced only in the regions close to the neutron star surface. We study how the magnetosphere transitions from the vacuum to…

High Energy Astrophysical Phenomena · Physics 2018-05-10 Gabriele Brambilla , Constantinos Kalapotharakos , Andrey Timokhin , Alice Harding , Demosthenes Kazanas

Mergers of neutron star-neutron star (NS-NS) or neutron star-black hole (NS-BH) binaries are candidate sources of gravitational waves (GWs). At least a fraction of the merger remnant should be a stellar mass BH with a sub-relativistic…

High Energy Astrophysical Phenomena · Physics 2018-01-10 Shuai-Bing Ma , Wei-Hua Lei , He Gao , Wei Xie , Wei Chen , Bing Zhang , Ding-Xiong Wang

We investigate electron--positron pair creation through the Schwinger process in newborn magnetars with millisecond spin periods and surface dipole fields close to or above the QED critical field, $B_{\rm Q} =…

High Energy Astrophysical Phenomena · Physics 2026-04-24 Chul Min Kim , Sang Pyo Kim , Remo Ruffini , Yu Wang , Shurui Zhang

I summarize recent results about how a neutron star binary coalescence can produce short gamma-ray bursts (GRBs). Two possibilities are discussed: the annihilation of neutrino anti-neutrino pairs above the merged remnant and the exponential…

Astrophysics · Physics 2010-11-11 S. Rosswog

Some active galactic nuclei, microquasars, and gamma ray bursts may be powered by the electromagnetic braking of a rapidly rotating black hole. We investigate this possibility via axisymmetric numerical simulations of a black hole…

Astrophysics · Physics 2008-11-26 Jonathan C. McKinney , Charles F. Gammie