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A facility to search for hidden particles at the CERN SPS: the SHiP physics case
TLDR
It is demonstrated that the SHiP experiment has a unique potential to discover new physics and can directly probe a number of solutions of beyond the standard model puzzles, such as neutrino masses, baryon asymmetry of the Universe, dark matter, and inflation.
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Ultrahigh-Energy Neutrino Interactions
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Prompt neutrino fluxes from atmospheric charm
We calculate the prompt neutrino flux from atmospheric charm production by cosmic rays, using the dipole picture in a perturbative QCD framework, which incorporates the parton saturation effects…
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Neutrino interactions at ultrahigh energies
We report new calculations of the cross sections for deeply inelastic neutrino-nucleon scattering at neutrino energies between 10{sup 9}thinspeV and 10{sup 21}thinspeV. We compare with results in the…
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The DUNE Far Detector Interim Design Report Volume 1: Physics, Technology and Strategies
The DUNE IDR describes the proposed physics program and technical designs of the DUNE Far Detector modules in preparation for the full TDR to be published in 2019. It is intended as an intermediate…
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Lepton fluxes from atmospheric charm
We reexamine the charm contribution to atmospheric lepton fluxes in the context of perturbative QCD. We include next-to-leading order corrections and discuss theoretical uncertainties due to the…
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High Energy Neutrino Cross Sections
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The POEMMA (Probe of Extreme Multi-Messenger Astrophysics) observatory
The Probe Of Extreme Multi-Messenger Astrophysics (POEMMA) is designed to accurately observe ultra-high-energy cosmic rays (UHECRs) and cosmic neutrinos from space with sensitivity over the full…
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Prompt atmospheric neutrino fluxes: perturbative QCD models and nuclear effects
A bstractWe evaluate the prompt atmospheric neutrino flux at high energies using three different frameworks for calculating the heavy quark production cross section in QCD: NLO perturbative QCD, kT…
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On the capture of dark matter by neutron stars
We calculate the number of dark matter particles that a neutron star accumulates over its lifetime as it rotates around the center of a galaxy, when the dark matter particle is a self-interacting…
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