2016
DOI: 10.1088/1367-2630/18/11/115006
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Instabilities of Weyl loop semimetals

Abstract: We study Weyl-loop semi-metals with short range interactions, focusing on the possible interaction driven instabilities. We introduce an ò expansion regularization scheme by means of which the possible instabilities may be investigated in an unbiased manner through a controlled weak coupling renormalization group (RG) calculation. The problem has enough structure that a 'functional' RG calculation (necessary for an extended Fermi surface) can be carried out analytically. The leading instabilities are identifie… Show more

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Cited by 44 publications
(42 citation statements)
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“…For example, the weak dispersion of the drumhead surface states leads to a large density of states near the Fermi level. Therefore, possible interaction-induced instabilities on the surface of nodal-line semimetals have been widely discussed in theory [12][13][14] .…”
Section: Introductionmentioning
confidence: 99%
“…For example, the weak dispersion of the drumhead surface states leads to a large density of states near the Fermi level. Therefore, possible interaction-induced instabilities on the surface of nodal-line semimetals have been widely discussed in theory [12][13][14] .…”
Section: Introductionmentioning
confidence: 99%
“…whereas the mass term m φ is not renormalized and can be set to zero at the fixed point, which corresponds to a quantum phase transition. We also note that the polarization bubble in the CDW, SC and SDW channels has explicit frequency dependence, and is distinct from earlier works that studied the effect of Coulomb interactions in the Yukawa language by decomposing the four fermion interaction in the Hartree channel [34,51]. In the Coulomb case, the bosonic propagator is frequency independent, implying in the absence of renormalization of the fermionic wavefunction.…”
Section: A One Loop Calculationsmentioning
confidence: 71%
“…In addition, Weyl SM (WSM), in which the low-energy fermionic excitations display linear dispersion around pairs of nodes with opposite chirality, was observed in TaAs, NbAs, TaP, and NbP by the angle-resolved photoemission spectroscopy (ARPES) [10][11][12][13][14]. There also exist other types of SMs, such as 3D nodal line SM (NLSM) [15][16][17][18], 2D semi-DSM , 3D double-WSM [47][48][49][50][51][52][53][54][55][56][57][58][59], 3D triple-WSM [49,53,[56][57][58][59][60][61][62], 3D anisotropic-WSM [49,[63][64][65], and 3D Luttinger SM [66][67][68][69][70].…”
Section: Introductionmentioning
confidence: 99%
“…The difference is owing to the fact that the fermion DOS vanishes at zero energy, namely ρ(0)=0. Cooper pairing instability may be achieved in other SMs, including 2D semi-DSM [43,44], 3D DSM [96], 3D WSM [97,98], 3D NLSM [17,18], and 3D Luttinger SM [67,69,70]. In these materials, there is also a threshold value for the strength of attraction.…”
Section: Introductionmentioning
confidence: 99%