About: Elena Amato

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An Entity of Type : wikibase:Item, within Data Space : wikidata.demo.openlinksw.com associated with source document(s)

researcher

Attributes	Values
rdf:type	Item
description	ikertzailea (eu) researcher (en) 연구원 (ko) 研究者 (ja) wetenschapper (nl) дослідниця (uk) эрдэмтэн (mn) वैज्ञानिक (hi) изилдөөчү (ky) 研究者 (zh) հետազոտող (hy) hulumtuese (sq)
rdfs:label	E. Amato (nl) E. Amato (ast) Elena Amato (en) Elena Amato (es) Elena Amato (it)
skos:prefLabel	E. Amato (nl) E. Amato (ast) Elena Amato (en) Elena Amato (es) Elena Amato (it)
name	E. Amato (nl) E. Amato (ast) Elena Amato (en) Elena Amato (es) Elena Amato (it)
Scopus author ID	wds:Q57094305-27E8F486-9570-40BD-B049-7CF25EB47D31
Scopus author ID	7003628769
given name	wds:Q57094305-A07DC3D5-AD8C-4A57-A858-1B994CC2F3B5
given name	Elena
instance of	wds:Q57094305-5445D28E-4E1C-4D6E-8E83-78F633F84240
instance of	Homo sapiens
zbMATH author ID	wds:Q57094305-00071DEF-F7B7-4A46-A3A1-56E218EB09B8
zbMATH author ID	amato.e
INSPIRE-HEP author ID	wds:Q57094305-A9E8594E-E17E-472D-AA5D-6CAECCA57150
INSPIRE-HEP author ID	E.Amato.1
skos:altLabel	E. Amato (en)
occupation	wds:Q57094305-BC940681-4980-48C9-944C-1A32C1BAAD23
employer	wds:Q57094305-7035C36A-0CED-4712-A5E1-499730AF4014
sex or gender	wds:Q57094305-6fe5f699-442a-e7bb-949b-d1a073d223d1
VIAF ID	wds:Q57094305-9A936C6E-DED9-4C87-9853-F5990BB617D2
IdRef ID	wds:Q57094305-44327e73-c1d3-4c3b-bf71-e9654d5ede98
maintained by WikiProject	wds:Q57094305-7036F9D2-86F8-42A9-AE6F-F3512E308A47
family name	wds:Q57094305-82DC7530-8F32-45A7-A122-A96B0E1E83CD
WorldCat Identities ID (superseded)	wds:Q57094305-32B555B0-8979-4AC3-A503-D7ADF2DDBB6C
VIAF ID	http://viaf.org/viaf/127153124373824492801
IdRef ID	http://www.idref.fr/242616976/id
occupation	researcher
employer	Arcetri Observatory
sex or gender	female organism
VIAF ID	127153124373824492801
IdRef ID	242616976
maintained by WikiProject	WikiProject Mathematics
family name	Amato
WorldCat Identities ID (superseded)	viaf-127153124373824492801
ORCID iD	wds:Q57094305-F48C21F3-E1C7-4C8A-8949-7274F66FF23F
ORCID iD	https://orcid.org/0000-0002-9881-8112
ORCID iD	0000-0002-9881-8112
ResearcherID	wds:Q57094305-AFEAD96C-9FB6-44D4-BEB0-DB1D95A9A345
ResearcherID	P-2938-2015
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q57094305
is author of	Introducing the CTA concept Diffusive propagation of cosmic rays from supernova remnants in the Galaxy. I: spectrum and chemical composition Diffusive propagation of cosmic rays from supernova remnants in the Galaxy. II: anisotropy Non-linear particle acceleration at non-relativistic shock waves in the presence of self-generated turbulence XIPE: the X-ray imaging polarimetry explorer Collisionless shocks in a partially ionized medium. III. Efficient cosmic ray acceleration Collisionless shocks in a partially ionized medium. I. Neutral return flux and its effects on acceleration of test particles Spectral Breaks as a Signature of Cosmic Ray Induced Turbulence in the Galaxy The fate of ultrahigh energy nuclei in the immediate environment of young fast-rotating pulsars The maximum momentum of particles accelerated at cosmic ray modified shocks A kinetic approach to cosmic-ray-induced streaming instability at supernova shocks Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout Neutrino flux predictions for galactic plerions Simulated synchrotron and Inverse Compton emission from Pulsar Wind Nebulae Revised Predictions of Neutrino Fluxes from Pulsar Wind Nebulae Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants Non-linear diffusive acceleration of heavy nuclei in supernova remnant shocks Modelling Jets, Tori and Flares in Pulsar Wind Nebulae Multi-D magnetohydrodynamic modelling of pulsar wind nebulae: recent progress and open questions Constraints on particle acceleration sites in the Crab nebula from relativistic magnetohydrodynamic simulations Modelling spectral evolution of pulsar wind nebulae inside supernova remnants Axially symmetric relativistic MHD simulations of Pulsar Wind Nebulae in Supernova Remnants. On the origin of torus and jet-like features Broad Balmer line emission and cosmic ray acceleration efficiency in supernova remnant shocks Cosmic ray acceleration and Balmer emission from SNR 0509-67.5 Collisionless shocks in a partially ionized medium. II. Balmer emission Supernova remnant W44: a case of cosmic-ray reacceleration The contribution of supernova remnants to the galactic cosmic ray spectrum Dynamical feedback of self-generated magnetic fields in cosmic ray modified shocks Gamma-ray emission from SNR RX J1713.7−3946 and the origin of galactic cosmic rays Dynamical Effects of Self-Generated Magnetic Fields in Cosmic-Ray-modified Shocks Signatures of high energy protons in pulsar winds Signature of Energy Losses on the Cosmic Ray Electron Spectrum Galactic observatory science with the ASTRI Mini-Array at the Observatorio del Teide On the magnetohydrodynamic modelling of the Crab nebula radio emission Cosmic ray acceleration and Balmer emission from RCW 86 (G315.4 – 2.3) A general solution to non-linear particle acceleration at non-relativistic shock waves

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