Radiation Field on Superspace

TL;DR

This paper explores the dynamics of multiwormhole configurations in string theory, proposing a modified Hamiltonian that introduces a radiation field on superspace influencing coupling constants.

Contribution

It introduces a novel modification to the Hamiltonian in string theory, enabling interpretation of Coleman parameters as a radiation field on superspace.

Findings

Planckian probability measure for Coleman parameters

Interpretation of $rac{1}{2}eta^{2}$ as radiation energy

Potential fixing of coupling constants by superspace radiation

Abstract

We study the dynamics of multiwormhole configurations within the framework of the Euclidean Polyakov approach to string theory, incorporating a modification to the Hamiltonian which leads to a Planckian probability measure for the Coleman parameters $\alpha$ that allows $\frac{1}{2}\alpha^{2}$ to be interpreted as the energy of the quanta of a radiation field on superspace whose values might still fix the coupling constants.