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Related papers: Optimal $\beta$-beam at the CERN-SPS

200 papers

In this paper we stress the idea that new, more precise neutrino cross-sections measurements at low energies will be necessary to improve the results of future big neutrino detectors, which will be dominated by the contribution of the…

High Energy Physics - Phenomenology · Physics 2008-11-26 M. Campanelli , S. Navas-Concha , A. Rubbia

The key process is the observation of tiny oscillation mixing between numu and nue related to so far unknown theta13 amplitude, at distances corresponding to an invariant neutrino flight path around about 2.0 MeV/km. Zucchelli [12] has…

High Energy Physics - Phenomenology · Physics 2007-05-23 Carlo Rubbia

We discuss the physics reach of $\beta$-Beams and $\nu$-Factories from a theoretical perspective, having as a guideline the problem of degeneracies. The presence of degenerate solutions in the measure of the neutrino oscillation parameters…

High Energy Physics - Phenomenology · Physics 2009-11-11 S. Rigolin

We apply Bayesian methods to study the sensitivity to neutrino masses of a Galactic supernova neutrino signal. Our procedure makes use of the full statistics of events and is remarkably independent of astrophysical assumptions. Present…

High Energy Physics - Phenomenology · Physics 2007-05-23 Enrico Nardi

We discuss the optimization of a neutrino factory experiment for neutrino oscillation physics in terms of muon energy, baselines, and oscillation channels (gold, silver, platinum). In addition, we study the impact and requirements for…

High Energy Physics - Phenomenology · Physics 2014-11-18 P. Huber , M. Lindner , M. Rolinec , W. Winter

The puzzle remains in the large discrepancy between neutron lifetime measured by the two distinct experimental approaches -- counts of beta decays in a neutron beam and storage of ultracold neutrons in a potential trap, namely, the beam…

Nuclear Experiment · Physics 2020-12-02 Wanchun Wei

The mass shift, width broadening, and spectral density for the $\omega$ meson in a heat bath of nucleons and pions is calculated using a general formula which relates the self-energy to the forward scattering amplitude. We use experimental…

Nuclear Theory · Physics 2009-11-10 A. T. Martell , P. J. Ellis

We introduce exposure as a means to making balanced comparisons of the sensitivities of long-baseline neutrino experiments to a nonzero \theta_{13}, to CP violation and to the neutrino mass hierarchy. We illustrate its use by comparing the…

High Energy Physics - Phenomenology · Physics 2008-11-26 V. Barger , Patrick Huber , Danny Marfatia , Walter Winter

The search for the Lepton Flavor Violating decay mu into e gamma will reach an unprecedented level of sensitivity within the next five years thanks to the MEG-II experiment. This experiment will take data at the Paul Scherrer Institut where…

High Energy Physics - Experiment · Physics 2018-01-25 G. Cavoto , A. Papa , F. Renga , E. Ripiccini , C. Voena

Our beam-beam parameter study using beam-beam simulations and PWFA (particle-driven plasma acceleration) beam parameters indicates that at 3 TeV, for examined electron beam lengths ${2~\mu\mathrm{m}\leq\sigma_z\leq 10~\mu\mathrm{m}}$, the…

Accelerator Physics · Physics 2020-10-05 Jian Bin Ben Chen , Daniel Schulte , Erik Adli

Considering the supersymmetric models with light neutralino and R-parity violation, we perform estimates of the signal rate expected at the recently proposed fixed target SHiP experiment exploiting CERN SPS beam of 400 GeV protons. We…

High Energy Physics - Phenomenology · Physics 2015-10-28 D. Gorbunov , I. Timiryasov

We calculate the sensitivity to nu_mu->nu_e appearance oscillations in various Fermilab main injector neutrino beam configurations using simulations of a MINOS-like detector and an OPERA-like detector. We make the assumption of 3 neutrino…

High Energy Physics - Phenomenology · Physics 2007-05-23 Lawrence Wai , Bradley Patterson

A water \v{C}erenkov detector project, of megaton scale, to be installed in the Fr\'ejus underground site and dedicated to nucleon decay, neutrinos from supernovae, solar and atmospheric neutrinos, as well as neutrinos from a super-beam…

The centrality dependence of thermal parameters, characterizing the hadron multiplicities, is determined phenomenologically for lead-on-lead collisions at CERN-SPS for a beam energy of 158 AGeV. The strangeness equilibration factor shows a…

Nuclear Theory · Physics 2008-11-26 J. Cleymans , B. Kampfer , S. Wheaton

We introduce a diagnostic -- the quantum noise fraction $\beta$ -- that determines the maximum sensitivity improvement achievable through quantum enhancement for any gravitational wave detector. Applied to the landscape of proposed…

General Relativity and Quantum Cosmology · Physics 2026-05-12 Sergio Gaudio

For the first time, we use the Gamma-ray Burst Monitor (GBM) on-board the Fermi satellite to search for sterile neutrino decay lines in the energy range 10-25 keV corresponding to sterile neutrino mass range 20-50 keV. This energy range has…

High Energy Astrophysical Phenomena · Physics 2015-02-12 Shunsaku Horiuchi , Kenny C. Y. Ng , Jennifer M. Gaskins , Miles Smith , Robert Preece

A non zero, surprisingly large value of the third mixing angle $\theta_{13}$ has been measured in reactor neutrino experiments. Currently the most precise measurement of $\sin^2 2\theta_{13}$ has been performed by the Daya Bay experiment…

High Energy Physics - Experiment · Physics 2013-02-12 Rupert Leitner

Nuclear double beta decay provides an extraordinarily broad potential to search for beyond Standard Model physics, probing already now the TeV scale, on which new physics should manifest itself. These possibilities are reviewed here. First,…

High Energy Physics - Experiment · Physics 2007-05-23 H. V. Klapdor-Kleingrothaus

We discuss the $\gamma$-ray emission of the radiogalaxy NGC 1275 (the central galaxy of the Perseus Cluster), detected by Fermi-LAT and MAGIC, in the framework of the "spine-layer" scenario, in which the jet is assumed to be characterized…

High Energy Astrophysical Phenomena · Physics 2015-06-19 F. Tavecchio , G. Ghisellini