Welcome to the new version of CaltechAUTHORS. Login is currently restricted to library staff. If you notice any issues, please email coda@library.caltech.edu
Published February 3, 2015 | Erratum + Submitted + Published
Journal Article Open

Yukawa Bound States of a Large Number of Fermions

Abstract

We consider the bound state problem for a field theory that contains a Dirac fermion x that Yukawa couples to a (light) scalar field ø. We are interested in bound states with a large number N of x particles. A Fermi gas model is used to numerically determine the dependence of the radius R of these bound states on N and also the dependence of the binding energy on N. Since scalar interactions with relativistic x's are suppressed two regimes emerge. For modest values of N the state is composed of non-relativistic x particles. In this regime as N increases R decreases. Eventually the core region becomes relativistic and the size of the state starts to increase as N increases. As a result, for fixed Yukawa coupling and x mass, there is a minimum sized state that occurs roughly at the value of N where the core region first becomes relativistic. As an application to dark matter, our analysis offers the possibility of having a supermassive thermal DM candidate. We also compute an elastic scattering form factor that can be relevant for direct detection if the dark matter is composed of such x particles.

Additional Information

© 2015 The Authors. This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited. Article funded by SCOAP3. Received: November 26, 2014; Accepted: January 15, 2015; Published: February 3, 2015. This work started from discussions with Natalia Toro who pointed out the suppression at high energies of Yukawa couplings and the form of the effective classical particle theory in Eq.(3). We are grateful to her for these key insights. This work is supported by the Gordon and Betty Moore Foundation through Grant No. 776 to the Caltech Moore Center for Theoretical Cosmology and Physics, and by the DOE Grant DE-SC0011632, and also by a DOE Early Career Award under Grant No. DE-SC0010255. We are also grateful for the support provided by the Walter Burke Institute for Theoretical Physics.

Attached Files

Published - art_10.1007_JHEP02_2015_023.pdf

Submitted - 1411.1772v1.pdf

Erratum - art_3A10.1007_2FJHEP10_282015_29165.pdf

Files

1411.1772v1.pdf
Files (1.2 MB)
Name Size Download all
md5:d162e99240260749314abb2687c33e2f
539.6 kB Preview Download
md5:af37ad2888f6ad15afa6efc2464a873a
132.9 kB Preview Download
md5:76bbcce70306076ac4f1d7f4ce01edde
500.4 kB Preview Download

Additional details

Created:
August 22, 2023
Modified:
October 23, 2023