Search Results - "Siegel, Daniel"
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GW170817 --the first observed neutron star merger and its kilonova: Implications for the astrophysical site of the r-process
Published in The European physical journal. A, Hadrons and nuclei (01-11-2019)“… The first neutron star (NS) merger observed by advanced LIGO and Virgo, GW170817, and its fireworks of electromagnetic counterparts across the entire…”
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Neutrino Fast Flavor Conversions in Neutron-Star Postmerger Accretion Disks
Published in Physical review letters (25-06-2021)“…A compact accretion disk may be formed in the merger of two neutron stars or of a neutron star and a stellar-mass black hole. Outflows from such accretion…”
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Three-dimensional GRMHD Simulations of Neutrino-cooled Accretion Disks from Neutron Star Mergers
Published in The Astrophysical journal (01-05-2018)“…Merging binaries consisting of two neutron stars (NSs) or an NS and a stellar-mass black hole typically form a massive accretion torus around the remnant black…”
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Collapsars as a major source of r-process elements
Published in Nature (London) (01-05-2019)“…The production of elements by rapid neutron capture (r-process) in neutron-star mergers is expected theoretically and is supported by multimessenger…”
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Three-Dimensional General-Relativistic Magnetohydrodynamic Simulations of Remnant Accretion Disks from Neutron Star Mergers: Outflows and r-Process Nucleosynthesis
Published in Physical review letters (08-12-2017)“…The merger of binary neutron stars, or of a neutron star and a stellar-mass black hole, can result in the formation of a massive rotating torus around a…”
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Jets from Neutron-Star Merger Remnants and Massive Blue Kilonovae
Published in Physical review letters (08-12-2023)“…We perform three-dimensional general-relativistic magnetohydrodynamic simulations with weak interactions of binary neutron-star (BNS) mergers resulting in a…”
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GRMHD Simulations of Neutron-star Mergers with Weak Interactions: r-process Nucleosynthesis and Electromagnetic Signatures of Dynamical Ejecta
Published in The Astrophysical journal (01-02-2023)“…Abstract Fast neutron-rich material ejected dynamically over ≲10 ms during the merger of a binary neutron star (BNS) can give rise to distinctive…”
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ELECTROMAGNETIC EMISSION FROM LONG-LIVED BINARY NEUTRON STAR MERGER REMNANTS. I. FORMULATION OF THE PROBLEM
Published in The Astrophysical journal (01-03-2016)“…ABSTRACT Binary neutron star (BNS) mergers are the leading model to explain the phenomenology of short gamma-ray bursts (SGRBs). Recent observations of…”
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ELECTROMAGNETIC EMISSION FROM LONG-LIVED BINARY NEUTRON STAR MERGER REMNANTS. II. LIGHT CURVES AND SPECTRA
Published in The Astrophysical journal (01-03-2016)“…ABSTRACT Recent observations indicate that in a large fraction of binary neutron star (BNS) mergers a long-lived neutron star (NS) may be formed rather than a…”
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Igniting Weak Interactions in Neutron Star Postmerger Accretion Disks
Published in The Astrophysical journal (01-11-2021)“…Abstract The merger of two neutron stars or a neutron star and a black hole typically results in the formation of a postmerger accretion disk. Outflows from…”
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The mind in psychotherapy: An interpersonal neurobiology framework for understanding and cultivating mental health
Published in Psychology and psychotherapy (01-06-2019)“…In this brief overview, I offer a conceptual approach to the mind that can support whatever clinical, research, public policy, or other approach you may be…”
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Three-dimensional General-relativistic Simulations of Neutrino-driven Winds from Rotating Proto-neutron Stars
Published in The Astrophysical journal (01-06-2022)“…Abstract We explore the effects of rapid rotation on the properties of neutrino-heated winds from proto-neutron stars (PNS) formed in core-collapse supernovae…”
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Transcranial red and near infrared light transmission in a cadaveric model
Published in PloS one (15-10-2012)“…Low level light therapy has garnered significant interest within the past decade. The exact molecular mechanisms of how red and near infrared light result in…”
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Recovery Schemes for Primitive Variables in General-relativistic Magnetohydrodynamics
Published in The Astrophysical journal (20-05-2018)“…General-relativistic magnetohydrodynamic (GRMHD) simulations are an important tool to study a variety of astrophysical systems such as neutron star mergers,…”
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Economic Analysis of a Noninvasive Molecular Pathologic Assay for Pigmented Skin Lesions
Published in JAMA dermatology (Chicago, Ill.) (01-09-2018)“…A recently described noninvasive gene expression test (the pigmented lesion assay [PLA]) with adhesive patch-based sampling has the potential to rule out…”
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Nuclear burning in collapsar accretion discs
Published in Monthly notices of the Royal Astronomical Society (01-12-2020)“…ABSTRACT The core collapse of massive, rapidly-rotating stars are thought to be the progenitors of long-duration gamma-ray bursts (GRB) and their associated…”
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An interpersonal neurobiology perspective on the mind and mental health: personal, public, and planetary well-being
Published in Annals of general psychiatry (03-02-2023)“…This article outlines an Interpersonal Neurobiology (IPNB) perspective on the fundamental components that comprise mental health and promote well-being. The…”
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Incidence and prevalence of basal cell carcinoma (BCC) and locally advanced BCC (LABCC) in a large commercially insured population in the United States: A retrospective cohort study
Published in Journal of the American Academy of Dermatology (01-11-2016)“…Background Accurate evaluation of basal cell carcinoma (BCC) in the United States was not possible before the 2011 release of BCC-specific International…”
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Three-dimensional General-relativistic Simulations of Neutrino-driven Winds from Magnetized Proto–Neutron Stars
Published in The Astrophysical journal (01-09-2023)“…Abstract Formed in the aftermath of a core-collapse supernova or neutron star merger, a hot proto–neutron star (PNS) launches an outflow driven by neutrino…”
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Machine learning and the future of Medicare fraud detection
Published in Journal of the American Academy of Dermatology (01-08-2020)Get full text
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