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1.
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The Forward Physics Facility at the High-Luminosity LHC
/ Feng, Jonathan L. (UC, Irvine) ; Kling, Felix (DESY) ; Reno, Mary Hall (Iowa U.) ; Rojo, Juan (NIKHEF, Amsterdam ; Vrije U., Amsterdam) ; Soldin, Dennis (Delaware U.) ; Anchordoqui, Luis A. (Lehman Coll.) ; Boyd, Jamie (CERN) ; Ismail, Ahmed (Oklahoma State U.) ; Harland-Lang, Lucian (Oxford U. ; Oxford U., Theor. Phys.) ; Kelly, Kevin J. (CERN) et al.
High energy collisions at the High-Luminosity Large Hadron Collider (LHC) produce a large number of particles along the beam collision axis, outside of the acceptance of existing LHC experiments. The proposed Forward Physics Facility (FPF), to be located several hundred meters from the ATLAS interaction point and shielded by concrete and rock, will host a suite of experiments to probe Standard Model (SM) processes and search for physics beyond the Standard Model (BSM) [...]
arXiv:2203.05090; UCI-TR-2022-01; CERN-PBC-Notes-2022-001; INT-PUB-22-006; BONN-TH-2022-04; FERMILAB-PUB-22-094-ND-SCD-T.-
Geneva : CERN, 2023-01-20 - 413 p.
- Published in : J. Phys. G 50 (2023) 030501
Fulltext: blank - PDF; 2203.05090 - PDF; FERMILAB-PUB-22-094-ND-SCD-T - PDF; Fulltext from Publisher: PDF; External links: Fermilab Library Server; eConf
In : 2021 Snowmass Summer Study, Seattle, WA, United States, 11 - 20 July 2021, pp.030501
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2.
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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
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3.
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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
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4.
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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
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5.
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Asymmetric dark matter: residual annihilations and self-interactions
/ Baldes, Iason (DESY) ; Cirelli, Marco (Paris, LPTHE) ; Panci, Paolo (CERN) ; Petraki, Kalliopi (Paris, LPTHE ; NIKHEF, Amsterdam) ; Sala, Filippo (DESY) ; Taoso, Marco (Madrid, IFT ; INFN, Turin)
Dark matter (DM) coupled to light mediators has been invoked to resolve the putative discrepancies between collisionless cold DM and galactic structure observations. However, $\gamma$-ray searches and the CMB strongly constrain such scenarios. [...]
arXiv:1712.07489; CERN-TH-2017-272; DESY-17-232; NIKHEF-2017-070.-
2018-06-26 - 9 p.
- Published in : SciPost Phys. 4 (2018) 041
Fulltext: fulltext1644396 - PDF; arXiv:1712.07489 - PDF;
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6.
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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
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7.
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Dark Matter's secret liaisons: phenomenology of a dark $U(1)$ sector with bound states
/ Cirelli, Marco (Paris, LPTHE) ; Panci, Paolo (CERN ; Paris, Inst. Astrophys.) ; Petraki, Kalliopi (Paris, LPTHE ; NIKHEF, Amsterdam) ; Sala, Filippo (Paris, LPTHE) ; Taoso, Marco (Madrid, IFT)
Dark matter (DM) charged under a dark U(1) force appears in many extensions of the Standard Model, and has been invoked to explain anomalies in cosmic-ray data, as well as a self-interacting DM candidate. In this paper, we perform a comprehensive phenomenological analysis of such a model, assuming that the DM abundance arises from the thermal freeze-out of the dark interactions. [...]
CERN-TH-2016-255; IFT-UAM-CSIC-16-144; NIKHEF-2016-062; arXiv:1612.07295.-
2017-05-18 - 36 p.
- Published in : JCAP 1705 (2017) 036
Fulltext: PDF;
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8.
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Gamma Rays from Top-Mediated Dark Matter Annihilations
/ Jackson, C.B. (Texas U., Arlington) ; Servant, Géraldine (CERN ; Barcelona, IFAE ; ICREA, Barcelona ; Saclay, SPhT) ; Shaughnessy, Gabe (Wisconsin U., Madison) ; Tait, Tim M.P. (UC, Irvine) ; Taoso, Marco (Saclay, SPhT ; British Columbia U.)
Lines in the energy spectrum of gamma rays are a fascinating experimental signal, which are often considered "smoking gun" evidence of dark matter annihilation. The current generation of gamma ray observatories are currently closing in on parameter space of great interest in the context of dark matter which is a thermal relic. [...]
arXiv:1303.4717.-
2013-07-08 - 24 p.
- Published in : JCAP 07 (2013) 006
Fulltext: PDF; External link: Preprint
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9.
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Gamma-ray lines and One-Loop Continuum from s-channel Dark Matter Annihilations
/ Jackson, C B (Texas U., Arlington) ; Servant, Geraldine (CERN ; IPhT, Saclay ; Barcelona, Autonoma U.) ; Shaughnessy, Gabe (Wisconsin U., Madison) ; Tait, Tim M P (UC, Irvine) ; Taoso, Marco (Barcelona, Autonoma U. ; British Columbia U.)
The era of indirect detection searches for dark matter has begun, with the sensitivities of gamma-ray detectors now approaching the parameter space relevant for weakly interacting massive particles. In particular, gamma ray lines would be smoking gun signatures of dark matter annihilation, although they are typically suppressed compared to the continuum. [...]
arXiv:1302.1802; CERN-PH-TH-2012-368.-
2013 - 32 p.
- Published in : JCAP 07 (2013) 021
External link: Preprint
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10.
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Effect of low mass dark matter particles on the Sun
/ Taoso, Marco ; Iocco, Fabio ; Meynet, Georges ; Bertone, Gianfranco ; Eggenberger, Patrick
We study the effect of dark matter (DM) particles in the Sun, focusing in particular on the possible reduction of the solar neutrinos flux due to the energy carried away by DM particles from the innermost regions of the Sun, and to the consequent reduction of the temperature of the solar core. We find that in the very low-mass range between 4 and 10 GeV, recently advocated to explain the findings of the DAMA and CoGent experiments, the effects on neutrino fluxes are detectable only for DM models with very small, or vanishing, self-annihilation cross section, such as the so-called asymmetric DM models, and we study the combination of DM masses and Spin Dependent cross sections which can be excluded with current solar neutrino data. [...]
arXiv:1005.5711.-
2010 - 14 p.
- Published in : Phys. Rev. D 82 (2010) 083509
External link: Preprint
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