We discuss first results of the search for K+ → π+vv from the 2016 data set of NA62. Standard model sensitivity is shown to be achieved. The experiment continued to take data in 2017 and 2018 and this data is currently under investigation. In addition, NA62 performs various searches for BSM particles which are sketched in this contribution.

First results from NA62 / Ambrosino, F.; Corvino, M.; Massarotti, P.; Mirra, M.; Napolitano, M.; Saracino, G.. - (2018), pp. 21-24. (Intervento presentato al convegno Proceedings of the 14th Patras Workshop on Axions, WIMPs and WISPs) [10.3204/DESY-PROC-2018-03/Dobrich_Babette].

First results from NA62

Ambrosino F.;Corvino M.;Massarotti P.;Napolitano M.;Saracino G.
2018

Abstract

We discuss first results of the search for K+ → π+vv from the 2016 data set of NA62. Standard model sensitivity is shown to be achieved. The experiment continued to take data in 2017 and 2018 and this data is currently under investigation. In addition, NA62 performs various searches for BSM particles which are sketched in this contribution.
2018
First results from NA62 / Ambrosino, F.; Corvino, M.; Massarotti, P.; Mirra, M.; Napolitano, M.; Saracino, G.. - (2018), pp. 21-24. (Intervento presentato al convegno Proceedings of the 14th Patras Workshop on Axions, WIMPs and WISPs) [10.3204/DESY-PROC-2018-03/Dobrich_Babette].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11588/822291
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