CERN Accelerating science

CERN Document Server 12 records found  1 - 10next  jump to record: Search took 0.62 seconds. 
1.
Cold atoms in space: community workshop summary and proposed road-map / Alonso, Iván (Balearic Islands U.) ; Alpigiani, Cristiano (Washington U., Seattle) ; Altschul, Brett (South Carolina U.) ; Araújo, Henrique (Imperial Coll., London) ; Arduini, Gianluigi (CERN) ; Arlt, Jan (Aarhus U.) ; Badurina, Leonardo (King's Coll. London) ; Balaž, Antun (Belgrade, Inst. Phys.) ; Bandarupally, Satvika (Florence U. ; INFN, Florence) ; Barish, Barry C. (LIGO Lab., Caltech) et al.
We summarize the discussions at a virtual Community Workshop on Cold Atoms in Space concerning the status of cold atom technologies, the prospective scientific and societal opportunities offered by their deployment in space, and the developments needed before cold atoms could be operated in space. The cold atom technologies discussed include atomic clocks, quantum gravimeters and accelerometers, and atom interferometers. [...]
arXiv:2201.07789; FERMILAB-CONF-22-694-V; CERN-TH-2022-004.- 2022-11-20 - 64 p. - Published in : EPJ Quant. Technol.: 9 (2022) , no. 1, pp. 30 Fulltext: bb4d1d31d6edd562e94939489bfc05d6 - PDF; 2201.07789 - PDF; Fulltext from Publisher: PDF; External link: Fermilab Library Server
2.
AEDGE: Atomic Experiment for Dark Matter and Gravity Exploration in Space / AEDGE Collaboration
We propose in this White Paper a concept for a space experiment using cold atoms to search for ultra-light dark matter, and to detect gravitational waves in the frequency range between the most sensitive ranges of LISA and the terrestrial LIGO/Virgo/KAGRA/INDIGO experiments. This interdisciplinary experiment, called Atomic Experiment for Dark Matter and Gravity Exploration (AEDGE), will also complement other planned searches for dark matter, and exploit synergies with other gravitational wave detectors. [...]
arXiv:1908.00802; KCL-PH-TH/2019-65; CERN-TH-2019-126.- 2020-03-04 - 25 p. - Published in : EPJ Quant. Technol. 7 (2020) 6 Fulltext: 1908.00802 - PDF; fermilab-pub-19-698-v - PDF; Fulltext from Publisher: PDF; External links: Open Access fulltext; Fermilab Library Server (fulltext available)
3.
High Energy Neutrino expectations from the Central Molecular Zone / Marinelli, Antonio (INFN, Pisa ; Pisa U.) ; Gaggero, Daniele (U. Amsterdam, GRAPPA) ; Grasso, Dario (INFN, Pisa ; Pisa U.) ; Taoso, Marco (Madrid, IFT) ; Urbano, Alfredo (CERN) ; Ventura, Sofia (INFN, Pisa ; Pisa U.)
The density of molecular gas in the central few hundreds parsecs of our Galaxy is estimated to be two orders of magnitude larger than the Galactic average. This, so called, Central Molecular Zone, represent a privileged target where to look for a signature of Galactic cosmic ray interactions. [...]
SISSA, 2018 - 8 p. - Published in : PoS ICRC2017 (2018) 939 Fulltext: PDF; External link: PoS server
In : 35th International Cosmic Ray Conference, Busan, Republique De Coree, 12 - 20 Jul 2017, pp.939
4.
Evidences of unconventional cosmic ray propagation in gamma-ray and neutrino astronomy / Grasso, Dario (INFN, Pisa ; Pisa U.) ; Gaggero, Daniele (U. Amsterdam, GRAPPA) ; Marinelli, Antonio (Pisa U. ; INFN, Pisa) ; Taoso, Marco (Madrid, Autonoma U.) ; Urbano, D (CERN) ; Valli, Mauro (INFN, Rome ; Rome U.)
Several independent analyses of Fermi-LAT results found evidences of a spatial dependence of the cosmic ray (CR) proton spectral index which is not accounted for conventional models of CR transport in the Galaxy. We show that these results may have a relevant impact on the gamma-ray and neutrino diffuse emissions of the Galaxy above the TeV. [...]
SISSA, 2017 - 5 p. - Published in : PoS NOW2016 (2017) 055 Fulltext: PDF; External link: PoS server
In : Neutrino Oscillation Workshop 2016, Otranto (lecce), Italy, 4 - 11 Sep 2016, pp.055
5.
The very high energy gamma-ray diffuse emission from the Galactic Center / Gaggero, Daniele (U. Amsterdam, GRAPPA) ; Grasso, Dario (INFN, Pisa ; Pisa U.) ; Marinelli, Antonio (Pisa U. ; INFN, Pisa) ; Taoso, Marco (Madrid, IFT) ; Urbano, Alfredo (CERN) ; Ventura, Sofia (INFN, Pisa ; Pisa U.)
We present a novel interpretation of the gamma-ray diffuse emission in the Galactic Center (GC) and the Central Molecular Zone (CMZ) regions. This is based on a scenario assuming a harder scaling of the diffusion coefficient with rigidity in the inner Galaxy which reproduces the radial dependence of the cosmic-ray (CR) spectral index recently inferred from Fermi-LAT. [...]
SISSA, 2018 - 5 p. - Published in : PoS EPS-HEP2017 (2017) 014 Fulltext: PDF; External link: PoS server
In : 2017 European Physical Society Conference on High Energy Physics, Venice, Italy, 05 - 12 Jul 2017, pp.014
6.
Hard Cosmic Ray Sea in the Galactic Center: a consistent interpretation of H.E.S.S. and Fermi-LAT $\gamma$-ray data / Gaggero, Daniele (U. Amsterdam, GRAPPA) ; Grasso, Dario (INFN, Pisa ; Pisa U.) ; Marinelli, Antonio (INFN, Pisa ; Pisa U.) ; Taoso, Marco (Madrid, IFT) ; Urbano, Alfredo (CERN) ; Ventura, Sofia (INFN, Pisa ; Pisa U.)
We present a novel interpretation of the gamma-ray diffuse emission measured by H.E.S.S. in the Galactic Center (GC) region and the Galactic ridge. [...]
arXiv:1707.08473.- SISSA, 2017-07-26 - 8 p. - Published in : PoS ICRC2017 (2018) 739 Fulltext: PoS(ICRC2017)739 - PDF; arXiv:1707.08473 - PDF; External links: PoS; PoS server
In : 35th International Cosmic Ray Conference, Busan, Republique De Coree, 12 - 20 Jul 2017, pp.739
7.
Interpretation of astrophysical neutrinos observed by IceCube experiment by setting Galactic and extra-Galactic spectral components / Marinelli, Antonio (INFN, Pisa ; Pisa U.) ; Gaggero, Daniele (Amsterdam U.) ; Grasso, Dario (INFN, Pisa ; Pisa U.) ; Urbano, Alfredo (CERN) ; Valli, Mauro (INFN, Trieste ; SISSA, Trieste)
The last IceCube catalog of High Energy Starting Events (HESE) obtained with a livetime of 1347 days comprises 54 neutrino events equally-distributed between the three families with energies between 25 TeV and few PeVs. Considering the homogeneous flavors distribution (1:1:1) and the spectral features of these neutrinos the IceCube collaboration claims the astrophysical origin of these events with more than $5\sigma$. [...]
arXiv:1604.05776.- 2016 - 4 p. - Published in : EPJ Web Conf. 116 (2016) 04009 External link: Preprint
8.
Gamma-ray and neutrino diffuse emissions of the Galaxy above the TeV / Gaggero, Daniele (U. Amsterdam, GRAPPA) ; Grasso, Dario (INFN, Pisa ; Pisa U.) ; Marinelli, Antonio (INFN, Pisa ; Pisa U.) ; Urbano, Alfredo (CERN) ; Valli, Mauro (INFN, Trieste ; SISSA, Trieste)
As recently shown, Fermi-LAT measurements of the diffuse gamma-ray emission from the Galaxy favor the presence of a smooth softening in the primary cosmic-ray spectrum with increasing Galactocentric distance. This result can be interpreted in terms of a spatial-dependent rigidity scaling of the diffusion coefficient. [...]
arXiv:1507.07796.- 2016 - Published in : J. Phys.: Conf. Ser. 718 (2016) 052018 External link: Preprint
9.
The gamma-ray and neutrino sky: a consistent picture of Fermi-LAT, H.E.S.S., Milagro, and IceCube results / Gaggero, Daniele (INFN, Pisa ; SISSA, Trieste ; U. Amsterdam, GRAPPA) ; Grasso, Dario (INFN, Pisa ; Pisa U.) ; Marinelli, Antonio (INFN, Pisa ; Pisa U.) ; Urbano, Alfredo (INFN, Trieste ; SISSA, Trieste ; CERN) ; Valli, Mauro (INFN, Trieste ; SISSA, Trieste)
In this Letter we propose a novel interpretation of the anomalous TeV gamma-ray diffuse emission observed by Milagro in the inner Galactic plane consistent with the signal reported by H.E.S.S. in the Galactic ridge; remarkably, our picture also accounts for a relevant portion of the neutrino flux measured by IceCube. [...]
arXiv:1504.00227.- 2015-12-16 - 5 p. - Published in : Astrophys. J. 815 (2015) L25 Preprint: PDF; External link: Preprint
10.
Constrained Simulations of the Magnetic Field in the Local Universe and the Propagation of UHECRs / Dolag, Klaus (Padua U., Astron. Dept.) ; Grasso, Dario (Pisa, Scuola Normale Superiore ; INFN, Pisa) ; Springel, Volker (Garching, Max Planck Inst.) ; Tkachev, Igor (CERN)
We use simulations of LSS formation to study the build-up of magnetic fields (MFs) in the ICM. Our basic assumption is that cosmological MFs grow in a MHD amplification process driven by structure formation out of a seed MF present at high z. [...]
astro-ph/0410419.- 2005 - 30 p. - Published in : JCAP 01 (2005) 009 Access to fulltext document: PDF; Fulltext: PDF; External link: JCAPA

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47 Grasso, D
2 Grasso, D T
3 Grasso, D.
5 Grasso, Daniela
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