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Low-energy effective field theories of fermion liquids and the mixed U ( 1 ) × R d anomaly

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PhysRevB.103.165126.pdf

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sword-2022-05-04T16:28:14.original.xml (130 B)
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Author(s)
Wen, Xiao-Gang
Date Issued
2021
Journal
Physical Review B
Publisher
American Physical Society (APS)
Citation
Wen, Xiao-Gang. 2021. "Low-energy effective field theories of fermion liquids and the mixed U ( 1 ) × R d anomaly." Physical Review B, 103 (16).
Version
Final published version
Abstract
In this paper we study gapless fermionic and bosonic systems in $d$-dimensional continuum space with $U(1)$ particle-number conservation and $\mathbb{R}^d$ translation symmetry. We write down low energy effective field theories for several gapless phases where $U(1)\times \mathbb{R}^d$ is viewed as internal symmetry. The $U(1)\times \mathbb{R}^d$ symmetry, when viewed as an internal symmetry, has a mixed anomaly, and the different effective field theories for different phases must have the same mixed anomaly. Such a mixed anomaly is proportional to the particle number density, and can be measured from the distribution of the total momentum $\boldsymbol{k}_\text{tot}$ for low energy many-body states (\ie how such a distribution is shifted by $U(1)$ symmetry twist $\boldsymbol{a}$), as well as some other low energy universal properties of the systems. In particular, we write down low energy effective field theory for Fermi liquid with infinite number of fields, in the presence of both real space magnetic field and $\boldsymbol{k}$-space "magnetic" field. The effective field theory also captures the mixed anomaly, which constraints the low energy dynamics, such as determine the volume of Fermi surface (which is another formulation of Luttinger-Ward-Oshikawa theorem).
MIT Department
Massachusetts Institute of Technology. Department of Physics
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Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
https://hdl.handle.net/1721.1/142329
DOI of Published Version
https://doi.org/10.1103/PHYSREVB.103.165126
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