Ben Margalit
0000-0001-8405-2649
University of California
23 papers found
Refreshing results…
Fast Radio Bursts from Magnetars Born in Binary Neutron Star Mergers and Accretion Induced Collapse
Multi-messenger EOS constraints using binary NS mergers
Multi-messenger Bayesian parameter inference of a binary neutron-star merger
The Multi-messenger Matrix: The Future of Neutron Star Merger Constraints on the Nuclear Equation of State
Nuclear-dominated accretion flows in two dimensions – II. Ejecta dynamics and nucleosynthesis for CO and ONe white dwarfs
A Radio Source Coincident with the Superluminous Supernova PTF10hgi: Evidence for a Central Engine and an Analog of the Repeating FRB 121102?
Fast radio bursts as synchrotron maser emission from decelerating relativistic blast waves
An Embedded X-Ray Source Shines through the Aspherical AT 2018cow: Revealing the Inner Workings of the Most Luminous Fast-evolving Optical Transients
Where is the Engine Hiding Its Missing Energy? Constraints from a Deep X-Ray Non-detection of the Superluminous SN 2015bn
A Concordance Picture of FRB 121102 as a Flaring Magnetar Embedded in a Magnetized Ion–Electron Wind Nebula
One Thousand Days of SN2015bn: HST Imaging Shows a Light Curve Flattening Consistent with Magnetar Predictions
Unveiling the engines of fast radio bursts, superluminous supernovae, and gamma-ray bursts
The GRB–SLSN connection: misaligned magnetars, weak jet emergence, and observational signatures
Constraining the Maximum Mass of Neutron Stars from Multi-messenger Observations of GW170817
Millisecond Magnetar Birth Connects FRB 121102 to Superluminous Supernovae and Long-duration Gamma-Ray Bursts
The GRB-SLSN Connection: mis-aligned magnetars, weak jet emergence, and observational signatures
Merger of a white dwarf–neutron star binary to 1029carat diamonds: origin of the pulsar planets
Time-dependent models of accretion discs with nuclear burning following the tidal disruption of a white dwarf by a neutron star
Inferring the distances of fast radio bursts through associated 21-cm absorption
Constraining MOND using the vertical motion of stars in the solar neighbourhood
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