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1.
Euclid. I. Overview of the Euclid mission / Euclid Collaboration
The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. [...]
arXiv:2405.13491. - 94.
Fulltext
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2.
Sensitivity projections for a dual-phase argon TPC optimized for light dark matter searches through the ionization channel / Global Argon Dark Matter Collaboration
Dark matter lighter than 10 GeV/c$^2$ encompasses a promising range of candidates. A conceptual design for a new detector, DarkSide-LowMass, is presented, based on the DarkSide-50 detector and progress toward DarkSide-20k, optimized for a low-threshold electron-counting measurement. [...]
arXiv:2209.01177.- 2023-06-01 - 19 p. - Published in : Phys. Rev. D 107 (2023) 112006 Fulltext: 2209.01177 - PDF; 91ce6168799b33f720d8ae133fe8e56d - PDF; External link: Fermilab Library Server
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3.
Separating $^{39}$Ar from $^{40}$Ar by cryogenic distillation with Aria for dark matter searches / DarkSide Collaboration
The Aria project consists of a plant, hosting a 350 m cryogenic isotopic distillation column, the tallest ever built, which is currently in the installation phase in a mine shaft at Carbosulcis S.p.A., Nuraxi-Figus (SU), Italy. Aria is one of the pillars of the argon dark-matter search experimental program, lead by the Global Argon Dark Matter Collaboration. [...]
arXiv:2101.08686.- 2021-04-26 - 18 p. - Published in : Eur. Phys. J. C 81 (2021) 359 Article from SCOAP3: PDF; Fulltext: PDF; Fulltext from Publisher: PDF;
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4.
Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos / DarkSide 20k Collaboration
Future liquid-argon DarkSide-20k and ARGO detectors, designed for direct dark matter search, will be sensitive also to core-collapse supernova neutrinos, via coherent elastic neutrino-nucleus scattering. This interaction channel is flavor-insensitive with a high-cross section, enabling for a high-statistics neutrino detection with target masses of $\sim$50~t and $\sim$360~t for DarkSide-20k and ARGO, respectively. [...]
arXiv:2011.07819.- 2021-03-15 - 22 p. - Published in : JCAP 2103 (2021) 043 Fulltext: 2011.07819 - PDF; fermilab-pub-20-601-nd-ppd - PDF; External link: Fermilab Library Server (fulltext available)
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5.
SiPM-matrix readout of two-phase argon detectors using electroluminescence in the visible and near infrared range / DarkSide Collaboration
Proportional electroluminescence (EL) in noble gases is used in two-phase detectors for dark matter searches to record (in the gas phase) the ionization signal induced by particle scattering in the liquid phase. The "standard" EL mechanism is considered to be due to noble gas excimer emission in the vacuum ultraviolet (VUV). [...]
arXiv:2004.02024; FERMILAB-PUB-20-155-PPD.- 2021-02-15 - 26 p. - Published in : Eur. Phys. J. C 81 (2021) 153 Article from SCOAP3: PDF; Fulltext: 2004.02024 - PDF; fermilab-pub-20-155-ppd - PDF; External link: Fermilab Library Server (fulltext available)
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6.
Design and construction of a new detector to measure ultra-low radioactive-isotope contamination of argon / DarkSide Collaboration
Large liquid argon detectors offer one of the best avenues for the detection of galactic weakly interacting massive particles (WIMPs) via their scattering on atomic nuclei. The liquid argon target allows exquisite discrimination between nuclear and electron recoil signals via pulse-shape discrimination of the scintillation signals. [...]
arXiv:2001.08106.- 2020-02-26 - 19 p. - Published in : JINST 15 (2020) P02024 Fulltext: fermilab-pub-20-023-ppd - PDF; 2001.08106 - PDF; Fulltext from Publisher: PDF; External link: Fermilab Library Server (fulltext available)
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7.
Time Delay and Inhomogeneities / De Ritis, R ; Covone, G ; Piedipalumbo, E
2002
In : 9th Marcel Grossmann Meeting on General Relativity, Rome, Italy, 2 - 8 Jul 2000, pp.2097-2098
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8.
Detecting Planets Beyond the Galaxy / Covone, G ; De Ritis, R
2002
In : 9th Marcel Grossmann Meeting on General Relativity, Rome, Italy, 2 - 8 Jul 2000, pp.2135-2136
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9.
Microlensing search towards M31 / Calchi Novati, S. ; Iovane, G. (Salerno U. ; INFN, Salerno) ; Marino, A.A. (Capodimonte Observ. ; INFN, Salerno) ; Auriere, M. (Midi-Pyrenees Observ.) ; Baillon, P. (CERN) ; Bouquet, A. (College de France) ; Bozza, V. (Salerno U. ; INFN, Salerno) ; Capaccioli, M. (Capodimonte Observ. ; INFN, Salerno) ; Capozziello, S. (Salerno U. ; INFN, Salerno) ; Cardone, V. (Salerno U. ; INFN, Salerno) et al.
We present the first results of the analysis of data collected during the 1998-99 observational campaign at the 1.3 meter McGraw-Hill Telescope, towards the Andromeda galaxy (M31), aimed to the detection of gravitational microlensing effects as a probe of the presence of dark matter in our and in M31 halo. The analysis is performed using the pixel lensing technique, which consists in the study of flux variations of unresolved sources and has been proposed and implemented by the AGAPE collaboration. [...]
astro-ph/0110706.- 2002 - 13 p. - Published in : Astron. Astrophys. 381 (2002) 848-861 Access to fulltext document: PDF; Fulltext: PDF; External link: astro-ph/0110706 PDF
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55 Covone, G
11 Covone, Giovanni
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