Subsystem complexity in warped AdS

被引:0
作者
Roberto Auzzi
Stefano Baiguera
Arpita Mitra
Giuseppe Nardelli
Nicolò Zenoni
机构
[1] Università Cattolica del Sacro Cuore,Dipartimento di Matematica e Fisica
[2] INFN — Sezione di Perugia,undefined
[3] Università degli studi di Milano Bicocca and INFN — Sezione di Milano-Bicocca,undefined
[4] TIFPA — INFN,undefined
[5] c/o Dipartimento di Fisica,undefined
[6] Università di Trento,undefined
[7] Indian Institute of Science Education and Research Bhopal,undefined
来源
Journal of High Energy Physics | / 2019卷
关键词
AdS-CFT Correspondence; Black Holes;
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摘要
We compute the ultraviolet divergences of holographic subregion complexity for the left and right factors of the thermofield double state in warped AdS3 black holes, both for the action and the volume conjectures. Besides the linear divergences, which are also present in the BTZ black hole, additional logarithmic divergences appear. For the action conjecture, these log divergences are not affected by the arbitrarity in the length scale associated with the counterterm needed to ensure reparameterization invariance. We find that the subregion action complexity obeys the superadditivity property for the thermofield double in warped AdS3, independently from the action counterterm coefficient. We study the temperature dependence of subregion complexity at constant angular momentum and we find that it is correlated with the sign of the specific heat.
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  • [1] Maldacena JM(2003)The black holes of topologically massive gravity JHEP 04 021-L283
  • [2] Hartman T(2013)undefined JHEP 05 014-undefined
  • [3] Maldacena J(2016)undefined Fortsch. Phys. 64 44-undefined
  • [4] Susskind L(2014)undefined Phys. Rev. D 90 126007-undefined
  • [5] Stanford D(2016)undefined Fortsch. Phys. 64 49-undefined
  • [6] Susskind L(2017)undefined JHEP 10 107-undefined
  • [7] Susskind L(2018)undefined Phys. Rev. Lett. 120 121602-undefined
  • [8] Jefferson R(2017)undefined Phys. Rev. D 96 126001-undefined
  • [9] Myers RC(2018)undefined JHEP 02 082-undefined
  • [10] Chapman S(2018)undefined Phys. Rev. D 98 126001-undefined