If heavy neutrinos with mass mνH≥2me are produced in the Sun via the decay 8B→8Be+e++νH in a side branch of pp-chain, they would undergo the observable decay into an electron, a positron and a light neutrino νH→νL+e++e−. In the present work Borexino data are used to set a bound on the existence of such decays. We constrain the mixing of a heavy neutrino with mass 1.5 MeV ≤mνH≤ 14 MeV to be |UeH|2≤(10−3−4×10−6) respectively. These are tighter limits on the mixing parameters than obtained in previous experiments at nuclear reactors and accelerators.
New limits on heavy sterile neutrino mixing in B8 decay obtained with the Borexino detector / Bellini, G.; Suvorov, Y.; Et, Al.. - In: PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. - ISSN 1550-7998. - 88:7(2013). [10.1103/PhysRevD.88.072010]
New limits on heavy sterile neutrino mixing in B8 decay obtained with the Borexino detector
Suvorov, Y.;
2013
Abstract
If heavy neutrinos with mass mνH≥2me are produced in the Sun via the decay 8B→8Be+e++νH in a side branch of pp-chain, they would undergo the observable decay into an electron, a positron and a light neutrino νH→νL+e++e−. In the present work Borexino data are used to set a bound on the existence of such decays. We constrain the mixing of a heavy neutrino with mass 1.5 MeV ≤mνH≤ 14 MeV to be |UeH|2≤(10−3−4×10−6) respectively. These are tighter limits on the mixing parameters than obtained in previous experiments at nuclear reactors and accelerators.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.