The role of the chemical potential in coupling superfluid dark matter to
baryons
T. Mistele. (2019)cite arxiv:1909.05710Comment: 20 pages.
Abstract
Superfluid dark matter postulates that the centers of galaxies contain
superfluid condensates. An important quantity regarding these superfluids is
their chemical potential $ $. Here, we discuss two issues related to this
chemical potential. First, there is no exactly conserved quantity associated
with this chemical potential due to the symmetry-breaking baryon-phonon
coupling. Second, $ $ is sometimes introduced by shifting the phonon field
by $ t $ which -- again due to the symmetry-breaking baryon-phonon
coupling -- introduces an explicit time dependence in the Lagrangian. We
investigate under which conditions introducing a chemical potential is
nevertheless justified and show how to correctly introduce it when these
conditions are met. We further propose a model that recovers superfluid dark
matter's zero-temperature equations of motion including a chemical potential
even if the aforementioned conditions for justifying a chemical potential are
not met.
Description
The role of the chemical potential in coupling superfluid dark matter to baryons
%0 Generic
%1 mistele2019chemical
%A Mistele, Tobias
%D 2019
%K capjc dark matter mond
%T The role of the chemical potential in coupling superfluid dark matter to
baryons
%U http://arxiv.org/abs/1909.05710
%X Superfluid dark matter postulates that the centers of galaxies contain
superfluid condensates. An important quantity regarding these superfluids is
their chemical potential $ $. Here, we discuss two issues related to this
chemical potential. First, there is no exactly conserved quantity associated
with this chemical potential due to the symmetry-breaking baryon-phonon
coupling. Second, $ $ is sometimes introduced by shifting the phonon field
by $ t $ which -- again due to the symmetry-breaking baryon-phonon
coupling -- introduces an explicit time dependence in the Lagrangian. We
investigate under which conditions introducing a chemical potential is
nevertheless justified and show how to correctly introduce it when these
conditions are met. We further propose a model that recovers superfluid dark
matter's zero-temperature equations of motion including a chemical potential
even if the aforementioned conditions for justifying a chemical potential are
not met.
@misc{mistele2019chemical,
abstract = {Superfluid dark matter postulates that the centers of galaxies contain
superfluid condensates. An important quantity regarding these superfluids is
their chemical potential $ \mu $. Here, we discuss two issues related to this
chemical potential. First, there is no exactly conserved quantity associated
with this chemical potential due to the symmetry-breaking baryon-phonon
coupling. Second, $ \mu $ is sometimes introduced by shifting the phonon field
by $ \mu \cdot t $ which -- again due to the symmetry-breaking baryon-phonon
coupling -- introduces an explicit time dependence in the Lagrangian. We
investigate under which conditions introducing a chemical potential is
nevertheless justified and show how to correctly introduce it when these
conditions are met. We further propose a model that recovers superfluid dark
matter's zero-temperature equations of motion including a chemical potential
even if the aforementioned conditions for justifying a chemical potential are
not met.},
added-at = {2019-09-13T07:31:04.000+0200},
author = {Mistele, Tobias},
biburl = {https://www.bibsonomy.org/bibtex/2707aa3cd854c6658fe31fedcde59f37d/bdasgupta},
description = {The role of the chemical potential in coupling superfluid dark matter to baryons},
interhash = {505edf0f432c399a0d0be32c1d382749},
intrahash = {707aa3cd854c6658fe31fedcde59f37d},
keywords = {capjc dark matter mond},
note = {cite arxiv:1909.05710Comment: 20 pages},
timestamp = {2019-09-13T07:31:04.000+0200},
title = {The role of the chemical potential in coupling superfluid dark matter to
baryons},
url = {http://arxiv.org/abs/1909.05710},
year = 2019
}