On the Radiation Problem of High Mass Stars

TL;DR

This paper applies a specialized gravitational theory to argue that high mass stars can form through accretion disks without significant issues, challenging traditional views on stellar formation.

Contribution

It introduces the Azimuthally Symmetric Theory of Gravitation to support the feasibility of high mass star formation via accretion disks.

Findings

High mass stars can form via accretion disks according to the theory.

The Azimuthally Symmetric Theory of Gravitation supports star formation models.

Traditional problems in high mass star formation are addressed by this theory.

Abstract

We use the Azimuthally Symmetric Theory of Gravitation (set-forth in arXiv:0912.2966 and further advanced in viXra:0911.0025) to argue that massive stars must be able to form via the accretion disk without much problems.