2017/09/28 by Ze-Nan Chen, Xian-Hui Ge, Shang-Yu Wu +3 · 1 citation
Mathematics · Physics and Astronomy · #Black Holes and Theoretical Physics #Condensed matter physics #Cosmology and Gravitation Theories #Electrical resistivity and conductivity #Exponent #Geometry #Hall effect #Holography #Horizon #Mathematics #Nernst effect #Nernst equation #Noncommutative and Quantum Gravity Theories #Physics #Quantum mechanics #Scaling #Seebeck coefficient #Spacetime #cond-mat.str-el #gr-qc #hep-th
paper · pdf · doi:10.1016/j.nuclphysb.2017.09.016
1+23 pages, 4 figures, references added
openalex publication_date 2017/09/28 · arxiv created 2017/10/27 · arxiv updated 2018/03/14 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We investigate an Einstein–Maxwell-Dilaton–Axion holographic model and obtain two branches of a charged black hole solution with a dynamic exponent and a hyperscaling violation factor when a magnetic field presents. The magnetothermoelectric DC conductivities are then calculated in terms of horizon data by means of holographic principle. We find that linear temperature dependence resistivity and quadratic temperature dependence inverse Hall angle can be achieved in our model. The well-known anomalous temperature scaling of the Nernst signal and the Seebeck coefficient of cuprate strange metals are also discussed.