about
Illuminating gravitational waves: A concordant picture of photons from a neutron star merger.A radio counterpart to a neutron star merger.Are ultra-long gamma-ray bursts caused by blue supergiant collapsars, newborn magnetars, or white dwarf tidal disruption events?Synchrotron Radiation from the Fast Tail of Dynamical Ejecta of Neutron Star MergersFrom γ to Radio: The Electromagnetic Counterpart of GW170817Implications of the radio and X-ray emission that followed GW170817Detecting Black Hole Binaries by GaiaA cocoon shock breakout as the origin of the γ-ray emission in GW170817The γ-rays that accompanied GW170817 and the observational signature of a magnetic jet breaking out of NS merger ejectaMagnetorotational Instability in Eccentric DisksThe cocoon emission – an electromagnetic counterpart to gravitational waves from neutron star mergersElectron-capture Isotopes Could Constrain Cosmic-Ray Propagation ModelsThe Extragalactic Ultra-high-energy Cosmic-Ray DipoleObservational evidence for mass ejection accompanying short gamma-ray burstsOptical Follow-up of Gravitational-wave Events with Las Cumbres ObservatoryImplications of the Low Binary Black Hole Aligned Spins Observed by LIGOProbing the Extragalactic Cosmic-Ray Origin with Gamma-Ray and Neutrino BackgroundsEvolution of Supernova Remnants Near the Galactic CenterThe observable signatures of GRB cocoonsThe effect of cooling on particle trajectories and acceleration in relativistic magnetic reconnectionr-PROCESS PRODUCTION SITES AS INFERRED FROM Eu ABUNDANCES IN DWARF GALAXIESRadio counterparts of compact binary mergers detectable in gravitational waves: a simulation for an optimized surveyNatal kicks and time delays in merging neutron star binaries: implications for r-process nucleosynthesis in ultra-faint dwarfs and in the Milky WayASASSN-14li: A MODEL TIDAL DISRUPTION EVENTBeaming of particles and synchrotron radiation in relativistic magnetic reconnectionThe B/C and sub-iron/iron cosmic ray ratio - further evidence in favor of the spiral-arm diffusion modelGRB 131014A: a laboratory for studying the thermal-like and non-thermal emissions in gamma-ray bursts, and the new L^nTh^_i_-E^nTh,rest^_peak,i_RelationICECUBE neutrinos and Lorentz invariance violation'Disk formation versus disk accretion--What powers tidal disruption events?
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description
onderzoeker
@nl
researcher ORCID ID = 0000-0002-7964-5420
@en
name
Tsvi Piran
@ast
Tsvi Piran
@en
Tsvi Piran
@es
Tsvi Piran
@nl
type
label
Tsvi Piran
@ast
Tsvi Piran
@en
Tsvi Piran
@es
Tsvi Piran
@nl
prefLabel
Tsvi Piran
@ast
Tsvi Piran
@en
Tsvi Piran
@es
Tsvi Piran
@nl
P106
P31
P496
0000-0002-7964-5420