# Prediction and detection potential of fusion neutrinos from nearby stars

## TL;DR

This paper models neutrino spectra from nearby stars within 10 parsecs, analyzing their potential detectability and contributions from specific stellar objects using detailed stellar models.

## Contribution

It provides the first detailed calculations of neutrino spectra from individual nearby stars and assesses their potential for detection.

## Key findings

- Neutrino fluxes from nearby stars are quantified.
- Certain stars may produce detectable neutrino signals.
- The contribution of specific stars like Alpha Centauri and Sirius A is significant.

## Abstract

The shapes of neutrino spectra and fluxes from representative stars in the solar neighborhood up to 10 pc are calculated. The individual contribution of the most important, specific stellar objects (the alpha-Centauri system, Sirius A, Procyon, Vega, Fomalhaut and Altair) are determined and investigated by detailed stellar modeling. The possibility for a potential detection is discussed.