activity
20082022
most citedAccretion disc dynamo activity in local simulations spanning weak-to-strong net vertical magnetic flux regimes

149 citations · 441 across the 11 of their papers we have counts for

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9 papers · 1 filter

astro-ph.HE2022★ 12 cited

An Electron-Scattering Time Delay in Black Hole Accretion Disks

Greg Salvesen

Universal to black hole X-ray binaries, the high-frequency soft lag gets longer during the hard-to-intermediate state transition, evolving from to ${\sim}10~…

astro-ph.HE2020★ 34 cited

Black Hole Spin in X-ray Binaries: Giving Uncertainties an

Greg Salvesen, Jonah M. Miller

The two established techniques for measuring black hole spin in X-ray binaries often yield conflicting results, which must be resolved before either method may be deemed robust. In…

astro-ph.HE2020★ 26 cited

Origin of Spin-Orbit Misalignments: The Microblazar V4641 Sgr

Greg Salvesen, Supavit Pokawanvit

Of the known microquasars, V4641 Sgr boasts the most severe lower limit (> 52°) on the misalignment angle between the relativistic jet axis and the binary orbital angular momentum.…

astro-ph.HE2017★ 25 cited

Convective Quenching of Field Reversals in Accretion Disc Dynamos

Matthew S. B. Coleman, Evan Yerger, Omer Blaes +2

Vertically stratified shearing box simulations of magnetorotational turbulence commonly exhibit a so-called butterfly diagram of quasi-periodic azimuthal field reversals. However,…

astro-ph.HE2016★ 38 cited

Strongly magnetized accretion discs require poloidal flux

Greg Salvesen, Philip J. Armitage, Jacob B. Simon +1

Motivated by indirect observational evidence for strongly magnetized accretion discs around black holes, and the novel theoretical properties of such solutions, we investigate how…

astro-ph.HE2015★ 149 cited

Accretion disc dynamo activity in local simulations spanning weak-to-strong net vertical magnetic flux regimes

Greg Salvesen, Jacob B. Simon, Philip J. Armitage +1

Strongly magnetized accretion discs around black holes have attractive features that may explain enigmatic aspects of X-ray binary behaviour. The structure and evolution of these d…

astro-ph.HE2013★ 46 cited

A physical model for state transitions in black hole X-ray binaries

Chris Nixon, Greg Salvesen

We present an accretion cycle which can explain state transitions and other observed phenomena in black hole X-ray binaries. This model is based on the process of disc tearing, whe…

astro-ph.HE2013★ 44 cited

Spectral hardening as a viable alternative to disc truncation in black hole state transitions

Greg Salvesen, Jon M. Miller, Rubens C. Reis +1

Constraining the accretion flow geometry of black hole binaries in outburst is complicated by the inability of simplified multi-colour disc models to distinguish between changes in…

astro-ph.HE2013★ 19 cited

Quantifying energetics and dissipation in magnetohydrodynamic turbulence

Greg Salvesen, Kris Beckwith, Jacob B. Simon +2

We perform a suite of two- and three-dimensional magnetohydrodynamic (MHD) simulations with the Athena code of the non-driven Kelvin-Helmholtz instability in the subsonic, weak mag…