activity
20142026
most citedGravitational-wave glitches in chaotic extreme-mass-ratio inspirals

82 citations · 873 across the 60 of their papers we have counts for

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34 papers · 1 filter

astro-ph.HE2026

Transient discs around isolated accreting neutron stars

Marina D. Afonina, Anton V. Biryukov, Sergei B. Popov +1

Mature, isolated neutron stars can accrete from the interstellar medium. Due to turbulence, the accreted gas can have a substantial angular momentum and form a disc around the comp…

astro-ph.HE2026

Population synthesis and detection prospects for Galactic long-period transients with LISA

Arthur G. Suvorov, Nikolaos Karnesis, Valeriya Korol

The recently-discovered long-period radio transients represent a puzzling new class of astrophysical sources, some of which are thought to be compact binary systems emitting a puls…

astro-ph.HE2026

Magnetorotational instabilities in solids: Application to neutron-star crusts

Arthur G. Suvorov, Thomas Celora, Kostas D. Kokkotas

The magnetorotational instability can generate strong, turbulent substructure within magnetized shear flows. The efficacy of the mechanism as a function of microphysical aspects of…

astro-ph.HE2026

Dynamics of magnetoviscous warped discs around compact objects

Arthur G. Suvorov, Kostas Glampedakis

Accretion discs that are tilted with respect to their compact hosts can warp out-of-plane through general relativistic frame-dragging. Warp influences disc dynamics in ways that ha…

astro-ph.HE2025★ 4 cited

General-relativistic magnetar magnetospheres in 3D with physics-informed neural networks

Petros Stefanou, Arthur G. Suvorov, José A. Pons

Magnetar phenomena are likely intertwined with the location and structure of magnetospheric currents. General-relativistic effects are important in shaping the force-free equilibri…

astro-ph.HE2025★ 3 cited

Revealing the nature of long-period transients with space-based gravitational-wave interferometers

Arthur G. Suvorov, Clara Dehman, José A. Pons

A few members of the recently discovered class of long-period transients have been identified as binaries with white-dwarf primaries. In most cases, however, electromagnetic data a…

astro-ph.HE2025★ 2 cited

Late-blooming magnetars: awakening as long period transients after a dormant cooling epoch

Arthur G. Suvorov, Clara Dehman, José A. Pons

Long-period transients are an elusive class of compact objects uncovered by radio surveys. While magnetars are a leading candidate for those sources that appear isolated, several o…

astro-ph.HE2025★ 1 cited

Non-linear saturation of gravito-inertial modes excited by tidal resonances in binary neutron stars

Alexis Reboul-Salze, Aurélie Astoul, Hao-Jui Kuan +1

During the last seconds of a binary neutron-star merger, the tidal force can excite stellar oscillation modes to large amplitudes. From the perspective of premerger electromagnetic…

astro-ph.HE2025★ 6 cited

Magnetar structure in non-linear electrodynamics with mixed poloidal-toroidal fields

Arthur G. Suvorov, José A. Pons

Magnetars have inferred polar field strengths in excess of the Schwinger limit, where non-linear electromagnetic effects can be significant. Their internal fields may be even stron…

astro-ph.HE2024★ 11 cited

Premerger phenomena in neutron-star binary coalescences

Arthur G. Suvorov, Hao-Jui Kuan, Kostas D. Kokkotas

A variety of high-energy events can take place in the seconds leading up to a binary neutron-star merger. Mechanisms involving tidal resonances, electrodynamic interactions, or sho…

astro-ph.HE2024

Couplings of torsional and shear oscillations in a neutron star crust

Hajime Sotani, Arthur G. Suvorov, Kostas D. Kokkotas

Mature neutron stars are thought to be sufficiently cold that nuclei in the outer layers freeze, solidifying a crust. Crustal elasticity allows the star to support a set of seismic…

astro-ph.HE2024★ 2 cited

Magnetic amplification in premerger neutron stars through resonance-induced magnetorotational instabilities

Arthur G. Suvorov, Hao-Jui Kuan, Alexis Reboul-Salze +1

Tidal resonances in the final seconds of a binary neutron-star inspiral can excite oscillation modes in one or both of the constituents to large amplitudes. Under favorable circums…

astro-ph.HE2023★ 7 cited

Measuring spin in coalescing binaries of neutron stars showing double precursors

Hao-Jui Kuan, Arthur G. Suvorov, Kostas D. Kokkotas

Gamma-ray bursts resulting from binary neutron-star mergers are sometimes preceded by precursor flares. These harbingers may be ignited by quasi-normal modes, excited by orbital re…

astro-ph.HE2023★ 8 cited

The radio shut-off, glitch, and X-ray burst in 1E 1547.0-5408 interpreted through magnetic reconfiguration

Arthur G. Suvorov

A short X-ray burst was observed from the radio-loud magnetar 1E 1547.0-5408 in 2022 April. Unusually however, the source stopped showing radio pulsations weeks prior…

astro-ph.HE2023★ 21 cited

Evolutionary implications of a magnetar interpretation for GLEAM-X J162759.5-523504.3

Arthur G. Suvorov, Andrew Melatos

The radio pulsar GLEAM-X J162759.5-523504.3 has an extremely long spin period ($P = 1091.17\, \mbox{s}$), and yet seemingly continues to spin down rapidly ($\dot{P} < 1.2 \times 10…

astro-ph.HE2022★ 8 cited

Does the gamma-ray binary LS I +61°303 harbor a magnetar?

Arthur G. Suvorov, Kostas Glampedakis

The high-mass X-ray binary LS I +61°303 is also cataloged as a gamma-ray binary as a result of frequent outbursts at TeV photon energies. The system has released two soft-gamma fla…

astro-ph.HE2022★ 22 cited

Quasi-periodic oscillations in precursor flares via seismic aftershocks from resonant shattering

Arthur G. Suvorov, Hao-Jui Kuan, Kostas D. Kokkotas

GRB 211211A was accompanied by a kilonova, implying a merger origin for the event. A precursor flare, modulated by quasi-periodic oscillations at $\approx 22\, \mbox{Hz}$, was also…

astro-ph.HE2021

Wave-optical effects in the microlensing of continuous gravitational waves by star clusters

Arthur G. Suvorov

Rapidly rotating neutron stars are promising sources for existing and upcoming gravitational-wave interferometers. While relatively dim, these systems are expected to emit continuo…

astro-ph.HE2021★ 12 cited

Modelling spin-up episodes in accreting millisecond X-ray pulsars

Kostas Glampedakis, Arthur G. Suvorov

Accreting millisecond X-ray pulsars are known to provide a wealth of physical information during their successive states of outburst and quiescence. Based on the observed spin-up a…

astro-ph.HE2021★ 12 cited

Magnetically supramassive neutron stars

Arthur G Suvorov, Kostas Glampedakis

It is commonly believed that neutron stars exceeding the maximum mass limit for stability could be formed in the aftermath of binary neutron star mergers, enjoying a short life of…

astro-ph.HE2021★ 25 cited

General-relativistic treatment of tidal -mode resonances in coalescing binaries of neutron stars. II. As triggers for precursor flares of short gamma-ray bursts

Hao-Jui Kuan, Arthur G. Suvorov, Kostas D. Kokkotas

In some short gamma-ray bursts, precursor flares occurring seconds prior to the main episode have been observed. These flares may then be associated with the last few cycles…

astro-ph.HE2021★ 28 cited

Ultra-compact X-ray binaries as dual-line gravitational-wave sources

Arthur G. Suvorov

By virtue of their sub-hour orbital periods, ultra-compact X-ray binaries are promising sources for the space-borne gravitational-wave interferometers LISA, Taiji, and TianQin. Som…

astro-ph.HE2021★ 27 cited

Precessing magnetars as central engines in short gamma-ray bursts

Arthur G. Suvorov, Kostas D. Kokkotas

Short gamma-ray bursts that are followed by long-duration X-ray plateaus may be powered by the birth, and hydrodynamic evolution, of magnetars from compact binary coalescence event…

astro-ph.HE2020★ 31 cited

Recycled pulsars with multipolar magnetospheres from accretion-induced magnetic burial

Arthur G. Suvorov, Andrew Melatos

Many millisecond pulsars are thought to be old neutron stars spun up (`recycled') during an earlier accretion phase. They typically have relatively weak ($\lesssim 10^{9} \text{ G}…