Electrical conductivity of strongly magnetized dense quark matter-possibility of quantum Hall effect

被引:5
|
作者
Dey, Jayanta [1 ]
Bandyopadhyay, Aritra [2 ,3 ]
Gupta, Akash [4 ]
Pujari, Naman [1 ]
Ghosh, Sabyasachi [1 ]
机构
[1] Indian Inst Technol Bhilai, GEC Campus, Raipur 492015, Chhattisgarh, India
[2] South China Normal Univ, Inst Quantum Matter, Guangdong Prov Key Lab Nucl Sci, Guangzhou 510006, Peoples R China
[3] South China Normal Univ, Southern Nucl Sci Comp Ctr, Guangdong Hong Kong Joint Lab Quantum Matter, Guangzhou 510006, Peoples R China
[4] Ludwig Maximilians Univ Munchen, Theresienstr 37, D-80333 Munich, Germany
关键词
Degenerate quark matter; Magnetic field; QHE and SdH; Conductivity and Resistivity; Neuron Star; TRANSPORT; FIELDS;
D O I
10.1016/j.nuclphysa.2023.122654
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
We have pointed out the possibilities of quantum Hall effect (QHE) and Shubnikov-de Haas (SdH) oscillation in the transportation of strongly magnetized degenerate quark matter- expected inside the highly dense compact star, such as the neutron star. The anisotropic pattern of electrical conductivity and resistivity tensor is explored in classical to quantum cases by considering the Landau quantization of quarks in the presence of a finite magnetic field. With increasing magnetic field, classical to quantum transitions are realized through enhanced (reduced) resistivity (conductivity) with QHE/SdH type oscillatory patterns. Estimating QCD relaxation time for degenerate quark matter from Ref. [57], eB approximate to (1 - 4)m2 pi can be considered a strong magnetic field for massless and degenerate quark matter with quark chemical potential mu approximate to 0.2 - 0.4 GeV. We discovered exotic quantum magnetic oscillating patterns associated with the QHE and SdH phenomena within the mentioned regimes.(c) 2023 Elsevier B.V. All rights reserved.
引用
收藏
页数:21
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