Zobrazeno 1 - 10
of 29
pro vyhledávání: '"Viviana Niro"'
Autor:
Valentina De Romeri, Enrique Fernandez-Martinez, Julia Gehrlein, Pedro A. N. Machado, Viviana Niro
Publikováno v:
Journal of High Energy Physics, Vol 2017, Iss 10, Pp 1-21 (2017)
Abstract The Inverse Seesaw naturally explains the smallness of neutrino masses via an approximate B − L symmetry broken only by a correspondingly small parameter. In this work the possible dynamical generation of the Inverse Seesaw neutrino mass m
Externí odkaz:
https://doaj.org/article/84eda5b522734584bee8aebdd4ff3ceb
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2021, 508 (2), pp.2204-2209. ⟨10.1093/mnras/stab2380⟩
Mon.Not.Roy.Astron.Soc., 2021, 508 (2), pp.2204-2209. ⟨10.1093/mnras/stab2380⟩
The gamma-ray emission of RX J1713–3946, despite being extensively studied in the GeV and TeV domains, remains poorly understood. This is mostly because, in this range, two competing mechanisms can efficiently produce gamma-rays: the inverse Compto
Autor:
Viviana Niro
Publikováno v:
J.Phys.Conf.Ser.
17th International Conference on Topics in Astroparticle and Underground Physics
17th International Conference on Topics in Astroparticle and Underground Physics, Aug 2021, Valencia, Spain. pp.012088, ⟨10.1088/1742-6596/2156/1/012088⟩
17th International Conference on Topics in Astroparticle and Underground Physics
17th International Conference on Topics in Astroparticle and Underground Physics, Aug 2021, Valencia, Spain. pp.012088, ⟨10.1088/1742-6596/2156/1/012088⟩
Among the galactic sources that can be detected by the KM3NeT detector, we will consider the eHWC J1825-134 source recently detected by the HAWC telescope. Moreover, we consider the source RX J1713.7-3946 and show the prospects of detection in a full
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c3e1457ee64309da3d30be018d025869
https://hal.science/hal-03588669
https://hal.science/hal-03588669
Autor:
Viviana Niro
Publikováno v:
PoS
37th International Cosmic Ray Conference
37th International Cosmic Ray Conference, Jul 2021, Berlin, Germany. pp.1215, ⟨10.22323/1.395.1215⟩
37th International Cosmic Ray Conference
37th International Cosmic Ray Conference, Jul 2021, Berlin, Germany. pp.1215, ⟨10.22323/1.395.1215⟩
International audience; The HAWC telescopes has recently revealed new spectra for gamma-ray sources in the Galactic plane. We will consider, in particular, the eHWC J1825-134 source and show the prospects to detect this source at the KM3NeT detector.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ad40193b31dd7730c4cf3458d8793e82
https://hal.archives-ouvertes.fr/hal-03373058
https://hal.archives-ouvertes.fr/hal-03373058
Publikováno v:
16th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories
16th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories, Jul 2021, Online, Italy. pp.2335-2344, ⟨10.1142/9789811269776_0181⟩
Astrophys.J.
PoS
37th International Cosmic Ray Conference
37th International Cosmic Ray Conference, Jul 2021, Berlin, Germany. pp.683, ⟨10.22323/1.395.0683⟩
Astrophys.J., 2021, 914 (2), pp.135. ⟨10.3847/1538-4357/abfda4⟩
16th Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories, Jul 2021, Online, Italy. pp.2335-2344, ⟨10.1142/9789811269776_0181⟩
Astrophys.J.
PoS
37th International Cosmic Ray Conference
37th International Cosmic Ray Conference, Jul 2021, Berlin, Germany. pp.683, ⟨10.22323/1.395.0683⟩
Astrophys.J., 2021, 914 (2), pp.135. ⟨10.3847/1538-4357/abfda4⟩
Recently, a diffuse emission of 1-100 GeV $\gamma$-rays has been detected from the direction of Andromeda. The emission is centered on the galaxy, and extends for $\sim 100-200$ kpc away from its center. Explaining the extended $\gamma-$ray emission
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bbf6a1d1c8702ec87c37dd83d091b9ff
https://hal.science/hal-03972467
https://hal.science/hal-03972467
Autor:
Viviana Niro
Publikováno v:
JINST
Postponed: 9th Very Large Volume Neutrino Telescope Workshop
Postponed: 9th Very Large Volume Neutrino Telescope Workshop, May 2021, Valencia, Spain. pp.C12004, ⟨10.1088/1748-0221/16/12/C12004⟩
Postponed: 9th Very Large Volume Neutrino Telescope Workshop
Postponed: 9th Very Large Volume Neutrino Telescope Workshop, May 2021, Valencia, Spain. pp.C12004, ⟨10.1088/1748-0221/16/12/C12004⟩
Among the sources detected by the HAWC telescope in the galactic plane, we will consider the eHWC J1825-134 source and show the prospects to detect this source at the KM3NeT detector. Moreover, we consider the prospects to detect the source RX J1713.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5bf523337b88ad51442daf4b523e250e
https://hal.archives-ouvertes.fr/hal-03482111
https://hal.archives-ouvertes.fr/hal-03482111
Publikováno v:
PoS
40th International Conference on High Energy Physics
40th International Conference on High Energy Physics, Jul 2020, Prague, Czech Republic. pp.599, ⟨10.22323/1.390.0599⟩
40th International Conference on High Energy Physics
40th International Conference on High Energy Physics, Jul 2020, Prague, Czech Republic. pp.599, ⟨10.22323/1.390.0599⟩
International audience; The HAWC telescope has recently revealed new spectra for gamma-ray sources in the Galactic plane. We will consider, with particular emphasis, the 2HWC J1825-134 source. Amongst the HAWC sources, it is indeed the most luminous
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aa219fd793c21662c3e376bc15de23b8
https://hal.science/hal-03210405
https://hal.science/hal-03210405
The eHWC J1825-134 gamma-ray source is located in the southern sky and has been recently detected by the HAWC observatory. Amongst the HAWC sources, it is the most luminous in the multi-TeV domain. We show the prospects to detect this source at the f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b62d12209e12a7ec84d23aff85f0b8ba
Autor:
Viviana Niro
Publikováno v:
Physical Review D
Physical Review D, American Physical Society, 2021, 103 (10), pp.103020. ⟨10.1103/PhysRevD.103.103020⟩
Phys.Rev.D
Phys.Rev.D, 2021, 103 (10), pp.103020. ⟨10.1103/PhysRevD.103.103020⟩
Physical Review D, American Physical Society, 2021, 103 (10), pp.103020. ⟨10.1103/PhysRevD.103.103020⟩
Phys.Rev.D
Phys.Rev.D, 2021, 103 (10), pp.103020. ⟨10.1103/PhysRevD.103.103020⟩
Among the gamma-ray sources detected by the HAWC observatory, we consider in details in this work the gamma-ray sources eHWC J1907+063 and eHWC J2019+368. These two sources belong to the three most luminous sources detected by HAWC, with emission abo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::337f0531db41b2e6751d7229e3024699
Publikováno v:
Phys.Rev.D
Phys.Rev.D, 2021, 104 (2), pp.023017. ⟨10.1103/PhysRevD.104.023017⟩
Physical Review D
Physical Review D, American Physical Society, 2021, 104 (2), pp.023017. ⟨10.1103/PhysRevD.104.023017⟩
Phys.Rev.D, 2021, 104 (2), pp.023017. ⟨10.1103/PhysRevD.104.023017⟩
Physical Review D
Physical Review D, American Physical Society, 2021, 104 (2), pp.023017. ⟨10.1103/PhysRevD.104.023017⟩
The eHWC J1825-134 source is located in the southern sky and has been recently detected by the HAWC observatory. It presents an hard spectral index and its gamma-ray flux extends up to energies close to 100 TeV without significant suppression. Amongs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a7b3ad1ff5641b9c5df688b9a113a93d
https://hal.archives-ouvertes.fr/hal-02371404
https://hal.archives-ouvertes.fr/hal-02371404