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Exotic Lifshitz transitions in topological materials

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arxiv 1701.06435 v3 pith:PWLZ6QJQ submitted 2017-01-23 cond-mat.other

classification cond-mat.other
keywords lifshitztopologicaltransitiontransitionsdiracdifferentfermilines
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abstract

Topological Lifshitz transitions involve many types of topological structures in momentum and frequency-momentum spaces: Fermi surfaces, Dirac lines, Dirac and Weyl points, etc. Each of these structures has their own topological invariant ($N_1$, $N_2$, $N_3$, $\tilde N_3$, etc.), which supports the stability of a given topological structure. The topology of the shape of Fermi surfaces and Dirac lines, as well as the interconnection of the objects of different dimensions, lead to numerous classes of Lifshitz transitions. The consequences of Lifshitz transitions are important in different areas of physics. The singularities emerging at the transition may enhance the transition temperature to superconductivity; the Lifshitz transition can be in the origin of the small masses of elementary particles in our Universe; the black hole horizon serves as the surface of Lifshitz transition between the vacua with type-I and type-II Weyl points; etc.

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Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Smart Holes: Analogue black holes with the right temperature and entropy

    hep-th 2024-12 conditional novelty 5.0 of 10

    The entropy of a tilted Dirac cone material, integrated across a spatially varying tilt, grows linearly with temperature behind the analogue horizon and can be mapped to BTZ black hole entropy.

  2. Black hole thermodynamics and topology

    gr-qc 2025-05 reject novelty 4.0 of 10

    The author derives S_RN = 4πM^2 for Reissner-Nordström black holes by adding the inverse temperatures of both horizons, contradicting the standard area law.

  3. Extended Tsallis-Cirto entropy for black and white holes

    gr-qc 2025-05 conditional novelty 4.0 of 10

    White hole entropy is proposed to be minus the black hole entropy of the same mass, and a modified composition rule makes charged black hole entropy depend only on mass.

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