Hořava-Lifshitz gravity and effective theory of the fractional quantum Hall effect

被引:0
|
作者
Chaolun Wu
Shao-Feng Wu
机构
[1] University of Chicago,Kadanoff Center for Theoretical Physics and Enrico Fermi Institute
[2] Shanghai University,Department of Physics
关键词
Gauge-gravity correspondence; Effective field theories; Holography and condensed matter physics (AdS/CMT);
D O I
暂无
中图分类号
学科分类号
摘要
We show that Hořava-Lifshitz gravity theory can be employed as a covariant framework to build an effective field theory for the fractional quantum Hall effect that respects all the spacetime symmetries such as non-relativistic diffeomorphism invariance and anisotropic Weyl invariance as well as the gauge symmetry. The key to this formalism is a set of correspondence relations that maps all the field degrees of freedom in the Hořava-Lifshitz gravity theory to external background (source) fields among others in the effective action of the quantum Hall effect, according to their symmetry transformation properties. We originally derive the map as a holographic dictionary, but its form is independent of the existence of holographic duality. This paves the way for the application of Hořava-Lifshitz holography on fractional quantum Hall effect. Using the simplest holographic Chern-Simons model, we compute the low energy effective action at leading orders and show that it captures universal electromagnetic and geometric properties of quantum Hall states, including the Wen-Zee shift, Hall viscosity, angular momentum density and their relations. We identify the shift function in Hořava-Lifshitz gravity theory as minus of guiding center velocity and conjugate to guiding center momentum. This enables us to distinguish guiding center angular momentum density from the internal one, which is the sum of Landau orbit spin and intrinsic (topological) spin of the composite particles. Our effective action shows that Hall viscosity is minus half of the internal angular momentum density and proportional to Wen-Zee shift, and Hall bulk viscosity is half of the guiding center angular momentum density.
引用
收藏
相关论文
共 50 条
  • [21] Mixmaster universe in the z = 3 deformed Hořava-Lifshitz gravity
    Yun Soo Myung
    Yong-Wan Kim
    Woo-Sik Son
    Young-Jai Park
    Journal of High Energy Physics, 2010
  • [22] Dynamical System Approach and Thermodynamical Perspective of Hořava-Lifshitz Gravity
    Samaddar, Amit
    Singh, S. Surendra
    FORTSCHRITTE DER PHYSIK-PROGRESS OF PHYSICS, 2024, 72 (06):
  • [24] Inflation in general covariant Hořava-Lifshitz gravity without projectability
    Tao Zhu
    Yongqing Huang
    Anzhong Wang
    Journal of High Energy Physics, 2013
  • [25] Cosmological test of dark energy parameterizations in Hořava-Lifshitz gravity
    Chaudhary, Himanshu
    Molla, Niyaz Uddin
    Khurana, Madhur
    Debnath, Ujjal
    Mustafa, G.
    EUROPEAN PHYSICAL JOURNAL C, 2024, 84 (03):
  • [26] U(1) Invariant F(R̀ƒ) Hořava-Lifshitz gravity
    Klusoň, J.
    Nojiri, S.
    Odintsov, S.D.
    Sáez-Gómez, D.
    European Physical Journal C, 2011, 71 (07): : 1 - 16
  • [27] Renormalization group flow of Hořava-Lifshitz gravity at low energies
    Adriano Contillo
    Stefan Rechenberger
    Frank Saueressig
    Journal of High Energy Physics, 2013
  • [28] Black Hole Entropy of IR Modified Hořava-Lifshitz Gravity in Quantum Statistics Perspective
    Molin Liu
    Junwang Lu
    Yonglei Jia
    Jianbo Lu
    International Journal of Theoretical Physics, 2011, 50 : 1978 - 1989
  • [29] Phantom energy accretion onto a black hole in Hořava-Lifshitz gravity
    G. Abbas
    Science China Physics, Mechanics and Astronomy, 2014, 57 : 604 - 607
  • [30] Gravitational Collapse with Dark Energy and Dark Matter in Hořava-Lifshitz Gravity
    Prabir Rudra
    Ujjal Debnath
    International Journal of Theoretical Physics, 2014, 53 : 2668 - 2687