collaborators

17 papers

astro-ph.HE20095 cited

Observable Signatures of the Accretion-Induced Collapse of White Dwarfs

B. D. Metzger, A. L. Piro, E. Quataert +1

Despite its probable occurrence in Nature, the accretion-induced collapse (AIC) of a white dwarf has not yet been directly observed (or, at least, it has not been unambiguously ide…

astro-ph.HE20095 cited

The Dynamic X-ray Sky of the Local Universe

Alicia M. Soderberg, Jonathan E. Grindlay, Joshua S. Bloom +35

Over the next decade, we can expect time domain astronomy to flourish at optical and radio wavelengths. In parallel with these efforts, a dedicated transient "machine" operating at…

astro-ph2008216 cited

Time-Dependent Models of Accretion Disks Formed from Compact Object Mergers

B. D. Metzger, A. L. Piro, E. Quataert

We present time-dependent models of the accretion disks created during compact object mergers, focusing on the energy available from accretion at late times and the composition of…

astro-ph200848 cited

Convection during the Late Stages of Simmering in Type Ia Supernovae

Anthony L. Piro, Philip Chang

Following unstable ignition of carbon, but prior to explosion, a white dwarf (WD) in a Type Ia supernova (SN Ia) undergoes a simmering phase. During this time, a central convective…

astro-ph2007

The Turbulent Story of X-ray Bursts: Effects of Shear Mixing on Accreting Neutron Stars

Anthony L. Piro, Lars Bildsten

During accretion, a neutron star (NS) is spun up as angular momentum is transported through its liquid surface layers. We study the resulting differentially rotating profile, focus…

astro-ph2006111 cited

Fragmentation of Collapsar Disks and the Production of Gravitational Waves

Anthony L. Piro, Eric Pfahl

We argue that gravitational instability in the outer parts of collapsar disks may lead to fragmentation near the radius where helium photodisintegrates, because of the strong cooli…