Search Results for author: Aaron C. Vincent

Found 6 papers, 5 papers with code

The Future of High-Energy Astrophysical Neutrino Flavor Measurements

no code implementations23 Dec 2020 Ningqiang Song, Shirley Weishi Li, Carlos A. Argüelles, Mauricio Bustamante, Aaron C. Vincent

We critically examine the ability of future neutrino telescopes, including Baikal-GVD, KM3NeT, P-ONE, TAMBO, and IceCube-Gen2, to determine the flavor composition of high-energy astrophysical neutrinos, ie, the relative number of $\nu_e$, $\nu_\mu$, and $\nu_\tau$, in light of improving measurements of the neutrino mixing parameters.

High Energy Physics - Phenomenology High Energy Astrophysical Phenomena

CosmoBit: A GAMBIT module for computing cosmological observables and likelihoods

1 code implementation7 Sep 2020 The GAMBIT Cosmology Workgroup, :, Janina J. Renk, Patrick Stöcker, Sanjay Bloor, Selim Hotinli, Csaba Balázs, Torsten Bringmann, Tomás E. Gonzalo, Will Handley, Sebastian Hoof, Cullan Howlett, Felix Kahlhoefer, Pat Scott, Aaron C. Vincent, Martin White

We introduce $\sf{CosmoBit}$, a module within the open-source $\sf{GAMBIT}$ software framework for exploring connections between cosmology and particle physics with joint global fits.

Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology

Strengthening the bound on the mass of the lightest neutrino with terrestrial and cosmological experiments

1 code implementation7 Sep 2020 The GAMBIT Cosmology Workgroup, :, Patrick Stöcker, Csaba Balázs, Sanjay Bloor, Torsten Bringmann, Tomás E. Gonzalo, Will Handley, Selim Hotinli, Cullan Howlett, Felix Kahlhoefer, Janina J. Renk, Pat Scott, Aaron C. Vincent, Martin White

We determine the upper limit on the mass of the lightest neutrino from the most robust recent cosmological and terrestrial data.

Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology

High-energy neutrino attenuation in the Earth and its associated uncertainties

1 code implementation29 Jun 2017 Aaron C. Vincent, Carlos A. Argüelles, Ali Kheirandish

We describe $\nu$FATE: Neutrino Fast Attenuation Through Earth, a very rapid method of accurately computing the attenuation of high-energy neutrinos during their passage through Earth to detectors such as IceCube, ANTARES or KM3Net, including production of secondary neutrinos from $\tau^\pm$ lepton decay.

High Energy Physics - Phenomenology High Energy Astrophysical Phenomena

Physics from solar neutrinos in dark matter direct detection experiments

1 code implementation4 Apr 2016 David G. Cerdeno, Malcolm Fairbairn, Thomas Jubb, Pedro A. N. Machado, Aaron C. Vincent, Celine Boehm

In this article, we compute the projected nuclear and electron recoil rates expected in several dark matter direct detection experiments due to solar neutrinos, and use these estimates to quantify errors on future measurements of the neutrino fluxes, weak mixing angle and solar observables, as well as to constrain new physics in the neutrino sector.

High Energy Physics - Phenomenology

Cannot find the paper you are looking for? You can Submit a new open access paper.