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of 5
pro vyhledávání: '"A. Sejersen Riis"'
Publikováno v:
In Astroparticle Physics March 2017 89:30-38
Publikováno v:
Hannen, V M, Heese, I, Weinheimer, C, Riis, A S & Valerius, K 2017, ' Deconvolution of the energy loss function of the KATRIN experiment ', Astroparticle Physics, vol. 89, pp. 30-38 . https://doi.org/10.1016/j.astropartphys.2017.01.010
The KATRIN experiment aims at a direct and model independent determination of the neutrino mass with 0.2 eV/c^2 sensitivity (at 90% C.L.) via a measurement of the endpoint region of the tritium beta-decay spectrum. The main components of the experime
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d50dbaf3bff79cefddb901d871456612
https://pure.au.dk/portal/da/publications/deconvolution-of-the-energy-loss-function-of-the-katrin-experiment(592afb24-ac5a-47a2-9f43-efa821dbed2a).html
https://pure.au.dk/portal/da/publications/deconvolution-of-the-energy-loss-function-of-the-katrin-experiment(592afb24-ac5a-47a2-9f43-efa821dbed2a).html
Publikováno v:
Riis, A S, Hannestad, S & Weinheimer, C 2011, ' Analysis of simulated data for the KArlsruhe TRItium Neutrino experiment using Bayesian inference ', Physical Review C (Nuclear Physics), vol. 84, no. 4, pp. id. 045503 . https://doi.org/10.1103/PhysRevC.84.045503
The KATRIN (Karlsruhe Tritium Neutrino) experiment will analyze the tritium $\ensuremath{\beta}$ spectrum to determine the mass of the neutrino with a sensitivity of $0.2$ eV (90$%$ C.L.). This approach to a measurement of the absolute value of the n
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::32573164bac925f5479c0765628a368a
https://doi.org/10.1103/physrevc.84.045503
https://doi.org/10.1103/physrevc.84.045503
Autor:
Anna Sejersen Riis, Steen Hannestad
Publikováno v:
Riis, A S & Hannestad, S 2011, ' Detecting sterile neutrinos with KATRIN like experiments ', Journal of Cosmology and Astroparticle Physics, vol. 02(2011)011 . https://doi.org/10.1088/1475-7516/2011/02/011
A sterile neutrino with mass in the eV range, mixing with the electron antineutrino, is allowed and possibly even preferred by cosmology and oscillation experiments. If such eV-mass neutrinos exist they provide a much better target for direct detecti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e6acad5dcd9afdaa0fce0560a8cae86c
http://arxiv.org/abs/1008.1495
http://arxiv.org/abs/1008.1495
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