CN-Cycle Neutrinos and Solar Metalicity

TL;DR

This paper explores the discrepancy between helioseismology and photospheric abundances in the Standard Solar Model, proposing a connection to giant planet formation and suggesting neutrino measurements to test solar core metalicity.

Contribution

It introduces a hypothesis linking solar model anomalies to planetary formation and proposes neutrino detection as a method to measure solar core metalicity.

Findings

Identifies a conflict in solar modeling data.

Suggests a link between solar composition and planetary formation.

Proposes neutrino measurements as a test for solar core metalicity.

Abstract

We discuss the current Standard Solar Model conflict between helioseismology and photospheric abundances, a speculation that connects this anomaly to formation of the gaseous giant planets, and a possible neutrino measurement to directly test solar core metalicity.