In February 2020, the Borexino Collaboration in collaboration with Tatsu Takeuchi, Sanjib Kumar Agarwalla and Chen Sun published [Journal of High Energy Physics 2 (2020) 038] the analysis of flavor-diagonal non-standard neutrino interactions (NSI) based on the Phase-II data.
Within the last few decades, solar neutrino physics has evolved into a field of relevance not only for probing our understanding of the Sun but also for investigating and determining intrinsic neutrino properties. Solar neutrinos can be utilized as a probe for new physics beyond the Standard Model that affect neutrino interactions with the charged leptons and quarks.
Monochromatic nature of the Be solar neutrinos results in an electron recoil spectrum whose shape is more sensitive to the couplings than that from a continuous neutrino energy spectrum. It gives an advantage in using the Sun as a neutrino source for the study of NSI’s.
In this paper, the neutrino-flavor-diagonal NSI’s that affect and interactions were investigated since Borexino is particularly sensitive to this set of parameters. The obtained bounds showed remarkable improvement, regardless of the choice of metallicity in the Standard Solar Model (SSM). The bounds are comparable to the global ones. In particular, the best constraint to-date on was obtained.
The same dataset, but without any NSI’s assumed, was used to measure , resulting in the value of (stat+syst). The precision is comparable to that measured by reactor antineutrino experiments.
This first sequence of plots (left panels of Figure 5 in our paper) shows the Log-likelihood profiles for the NSI parameters (red line) and (blue line) assuming HZ and LZ SSM’s.
This sequence of plots (right panels of Figure 5 in our paper) shows the Log-likelihood profiles for the NSI parameters (red line) and (blue line) assuming HZ and LZ SSM’s.
The one-dimensional profiles were obtained considering one NSI parameter at-a-time, while remaining NSI parameters were fixed to zero.
In this plot (Figure 6 of the paper), we report the allowed region for NSI parameters in plane. The bounds from LSND and TEXONO are provided for comparison. The contour obtained from the global analysis of solar neutrino experiments is presented by a dashed black line. Each contribution can be downloaded at the following links: TEXONO_top contour and TEXONO_bottom contour; LSND contour; Solar-KamLand contour; -HZ_Borexino contour; -LZ_Borexino contour.
The plot above (Figure 7 of our paper) shows the allowed region for NSI parameters in plane obtained in the present work. The contour from LEP is provided for comparison. Each contribution can be downloaded at the following links: -HZ_Borexino contour, -LZ_Borexino_right contour, -LZ_Borexino_left contour, LEP contour.