Neutrino Masses from Generalized Symmetry Breaking

Abstract

We explore generalized global symmetries in theories of physics beyond the standard model. Theories of <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"> <a:msup> <a:mi>Z</a:mi> <a:mo>′</a:mo> </a:msup> </a:math> bosons generically contain “noninvertible” chiral symmetries, whose presence indicates a natural paradigm to break this symmetry by an exponentially small amount in an ultraviolet completion. For example, in models of gauged lepton family difference such as the phenomenologically well motivated <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"> <c:mi mathvariant="normal">U</c:mi> <c:mo stretchy="false">(</c:mo> <c:mn>1</c:mn> <c:msub> <c:mo stretchy="false">)</c:mo> <c:mrow> <c:msub> <c:mi>L</c:mi> <c:mi>μ</c:mi> </c:msub> <c:mo>−</c:mo> <c:msub> <c:mi>L</c:mi> <c:mi>τ</c:mi> </c:msub> </c:mrow> </c:msub> </c:math> , there is a noninvertible lepton number symmetry which protects neutrino masses. We embed these theories in gauged non-Abelian horizontal lepton symmetries, e.g., <h:math xmlns:h="http://www.w3.org/1998/Math/MathML" display="inline"> <h:mi mathvariant="normal">U</h:mi> <h:mo stretchy="false">(</h:mo> <h:mn>1</h:mn> <h:msub> <h:mo stretchy="false">)</h:mo> <h:mrow> <h:msub> <h:mi>L</h:mi> <h:mi>μ</h:mi> </h:msub> <h:mo>−</h:mo> <h:msub> <h:mi>L</h:mi> <h:mi>τ</h:mi> </h:msub> </h:mrow> </h:msub> <h:mo>⊂</h:mo> <h:mrow> <h:mi>SU</h:mi> </h:mrow> <h:mo stretchy="false">(</h:mo> <h:mn>3</h:mn> <h:msub> <h:mo stretchy="false">)</h:mo> <h:mi>H</h:mi> </h:msub> </h:math> , where the generalized symmetries are broken nonperturbatively by the existence of lepton family magnetic monopoles. In such theories, either Majorana or Dirac neutrino masses may be generated through quantum gauge theory effects from the charged lepton Yukawas, e.g., <o:math xmlns:o="http://www.w3.org/1998/Math/MathML" display="inline"> <o:msub> <o:mi>y</o:mi> <o:mi>ν</o:mi> </o:msub> <o:mo>∼</o:mo> <o:msub> <o:mi>y</o:mi> <o:mi>τ</o:mi> </o:msub> <o:mi>exp</o:mi> <o:mo stretchy="false">(</o:mo> <o:mo>−</o:mo> <o:msub> <o:mi>S</o:mi> <o:mrow> <o:mi>inst</o:mi> </o:mrow> </o:msub> <o:mo stretchy="false">)</o:mo> </o:math> . These theories require no bevy of new fields nor additional global symmetries but are instead simple, natural, and predictive: The discovery of a lepton family <s:math xmlns:s="http://www.w3.org/1998/Math/MathML" display="inline"> <s:msup> <s:mi>Z</s:mi> <s:mo>′</s:mo> </s:msup> </s:math> at low energies will reveal the scale at which <u:math xmlns:u="http://www.w3.org/1998/Math/MathML" display="inline"> <u:msub> <u:mi>L</u:mi> <u:mi>μ</u:mi> </u:msub> <u:mo>−</u:mo> <u:msub> <u:mi>L</u:mi> <u:mi>τ</u:mi> </u:msub> </u:math> emerges from a larger gauge symmetry. Published by the American Physical Society 2024