Ab initio calculations of nuclear widths via an integral relation
Kenneth M. Nollett

TL;DR
This paper presents a new ab initio integral method to accurately compute nuclear state widths, improving agreement with experimental data for light nuclei and providing insights into state identification.
Contribution
Introduces an integral relation-based approach for calculating nuclear widths from variational Monte Carlo wave functions, enhancing accuracy over traditional spectroscopic factor estimates.
Findings
Predicted widths closely match experimental data for nuclei with 5 <= A <= 9.
Method identifies cases where computed widths are unreliable due to broad states.
Overlap functions can diagnose the trustworthiness of width calculations.
Abstract
I describe the computation of energy widths of nuclear states using an integral over the interaction region of ab initio variational Monte Carlo wave functions, and I present calculated widths for many states. I begin by presenting relations that connect certain short-range integrals to widths. I then present predicted widths for 5 <= A <= 9 nuclei, and I compare them against measured widths. They match the data more closely and with less ambiguity than estimates based on spectroscopic factors. I consider the consequences of my results for identification of observed states in ^8B, ^9He, and ^9Li. I also examine failures of the method and conclude that they generally involve broad states and variational wave functions that are not strongly peaked in the interaction region. After examining bound-state overlap functions computed from a similar integral relation, I conclude that overlap…
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