activity
20122026
most citedBlack holes, gravitational waves and fundamental physics: a roadmap

742 citations · 7.6k across the 81 of their papers we have counts for

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Showing astro-ph.SRShow all

9 papers · 1 filter

astro-ph.SR2020★ 88 cited

Observational constraints on the optical and near-infrared emission from the neutron star-black hole binary merger S190814bv

K. Ackley, L. Amati, C. Barbieri +151

On 2019 August 14, the LIGO and Virgo interferometers detected a high-significance event labelled S190814bv. Preliminary analysis of the GW data suggests that the event was likely…

astro-ph.SR2019★ 62 cited

PUSHing core-collapse supernovae to explosions in spherical symmetry IV: Explodability, remnant properties and nucleosynthesis yields of low metallicity stars

Kevin Ebinger, Sanjana Curtis, Somdutta Ghosh +5

In this fourth paper of the series, we use the parametrized, spherically symmetric explosion method PUSH to perform a systematic study of two sets of non-rotating stellar progenito…

astro-ph.SR2018★ 117 cited

PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry III: Nucleosynthesis Yields

Sanjana Curtis, Kevin Ebinger, Carla Fröhlich +4

In a previously presented proof-of-principle study, we established a parametrized spherically symmetric explosion method (PUSH) that can reproduce many features of core-collapse su…

astro-ph.SR2018★ 89 cited

PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry II: Explodability and Global Properties

Kevin Ebinger, Sanjana Curtis, Carla Fröhlich +4

In a previously presented proof-of-principle study we established a parametrized spherically symmetric explosion method (PUSH) that can reproduce many features of core-collapse sup…

astro-ph.SR2017★ 5 cited

PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry: Nucleosynthesis Yields

Sanjana Sinha, Carla Fröhlich, Kevin Ebinger +5

Core-collapse supernovae (CCSNe) are the extremely energetic deaths of massive stars. They play a vital role in the synthesis and dissemination of many heavy elements in the univer…

astro-ph.SR2015

Nucleosynthesis in the Ejecta of Neutron Star Mergers

Dirk Martin, Albino Perego, Almudena Arcones +2

Heavy elements like gold, platinum or uranium are produced in the r-process, which needs neutron-rich and explosive environments. Neutron star mergers are a promising candidate for…

astro-ph.SR2015★ 265 cited

Neutrino-driven winds in the aftermath of a neutron star merger: nucleosynthesis and electromagnetic transients

Dirk Martin, Albino Perego, Almudena Arcones +3

We present a comprehensive nucleosynthesis study of the neutrino-driven wind in the aftermath of a binary neutron star merger. Our focus is the initial remnant phase when a massive…

astro-ph.SR2015★ 114 cited

Pushing 1D CCSNe to explosions: model and SN 1987A

A. Perego, M. Hempel, C. Fröhlich +5

We report on a method, PUSH, for triggering core-collapse supernova explosions of massive stars in spherical symmetry. We explore basic explosion properties and calibrate PUSH such…

astro-ph.SR2012★ 558 cited

Magnetorotationally driven Supernovae as the origin of early galaxy -process elements?

Christian Winteler, Roger Kaeppeli, Albino Perego +5

We examine magnetorotationally driven supernovae as sources of -process elements in the early Galaxy. On the basis of thermodynamic histories of tracer particles from a three-di…