Publication data of Shaviv, Nir J.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion19952000200520102015202020250500100015002000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications19952000200520102015202020250153045607501.22.43.64.86
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion19952000200520102015202020250510152025
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestFireballs in dense stellar regions as an explanation of gamma-ray burstsCosmic ray diffusions from the galactic spiral arms, iron meteorites, and a possible climatic connectionsCosmic ray diffusions from the galactic spiral arms, iron meteorites, and a po…Magnetic lensing near ultramagnetized neutron starsLife extinctions by cosmic ray jetsThe nature of the radiative hydrodynamic instabilities in radiatively supported thomson atmospheresThe nature of the radiative hydrodynamic instabilities in radiatively supporte…PTF 13efv - An outburst 500 days prior to the SNHunt 275 explosion and its radiative efficiencyPTF 13efv - An outburst 500 days prior to the SNHunt 275 explosion and its …The Spiral structure of the Milky Way, cosmic rays, and ice age epochs on EarthThe Spiral structure of the Milky Way, cosmic rays, and ice age epochs on Ea…Origin of the high-energy extragalactic diffuse gamma-ray backgroundThe Origin of the binary pulsar J0737-3039BThe porous atmosphere of eta carinaeThe high-energy polarization-limiting radius of neutron star magnetospheres. 1. Slowly rotating neutron starsThe high-energy polarization-limiting radius of neutron star magnetospheres.…The theory of steady state super-eddington winds and its application to novaeQED and the high polarization of the thermal radiation from neutron starsPolarization evolution in strong magnetic fieldsSuper Eddington Slim Accretion Disks with WindsA Porosity-length formalism for photon-tiring-limited mass loss from stars above the Eddington limitA Porosity-length formalism for photon-tiring-limited mass loss from stars abo…Gamma-ray bursts from mini - jetsNatural explanation for the anomalous positron to electron ratio with supernova remnants as the sole cosmic ray sourceNatural explanation for the anomalous positron to electron ratio with superno…Precursors prior to Type IIn supernova explosions are common: precursor rates, properties, and correlationsPrecursors prior to Type IIn supernova explosions are common: precursor rat…19952000200520102015202020250500100015002000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Fireballs in dense stellar regions as an explanation of gamma-ray burstsCosmic ray diffusions from the galactic spiral arms, iron meteorites, and a possible climatic connectionsCosmic ray diffusions from the galactic spiral arms, iron meteorites, and a po…Magnetic lensing near ultramagnetized neutron starsLife extinctions by cosmic ray jetsThe nature of the radiative hydrodynamic instabilities in radiatively supported thomson atmospheresThe nature of the radiative hydrodynamic instabilities in radiatively supporte…PTF 13efv - An outburst 500 days prior to the SNHunt 275 explosion and its radiative efficiencyPTF 13efv - An outburst 500 days prior to the SNHunt 275 explosion and its …The Spiral structure of the Milky Way, cosmic rays, and ice age epochs on EarthThe Spiral structure of the Milky Way, cosmic rays, and ice age epochs on Ea…Origin of the high-energy extragalactic diffuse gamma-ray backgroundThe Origin of the binary pulsar J0737-3039BThe porous atmosphere of eta carinaeThe high-energy polarization-limiting radius of neutron star magnetospheres. 1. Slowly rotating neutron starsThe high-energy polarization-limiting radius of neutron star magnetospheres.…The theory of steady state super-eddington winds and its application to novaeQED and the high polarization of the thermal radiation from neutron starsPolarization evolution in strong magnetic fieldsSuper Eddington Slim Accretion Disks with WindsA Porosity-length formalism for photon-tiring-limited mass loss from stars above the Eddington limitA Porosity-length formalism for photon-tiring-limited mass loss from stars abo…Gamma-ray bursts from mini - jetsNatural explanation for the anomalous positron to electron ratio with supernova remnants as the sole cosmic ray sourceNatural explanation for the anomalous positron to electron ratio with superno…Precursors prior to Type IIn supernova explosions are common: precursor rates, properties, and correlationsPrecursors prior to Type IIn supernova explosions are common: precursor rat…19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average19952000200520102015202020250255075100125150