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Quantum Quench and Thermalization in Free Scalar Field Theory and its Gravity Dual (In Arbitrary Dimensions)

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dc.contributor.advisor Mandal, Gautam en_US
dc.contributor.author BANERJEE, PARIJAT en_US
dc.date.accessioned 2018-05-24T10:37:50Z
dc.date.available 2018-05-24T10:37:50Z
dc.date.issued 2018-05 en_US
dc.identifier.uri http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/1046
dc.description.abstract In this work we explore the thermalization of two point functions of free scalars in $d+1$ dimensions after a quantum quench. The mass is time dependent and is taken to zero. A detailed analysis of this problem has been done in 1+1 dimensions, in \cite{Mandal:2015kxi}. My goal here is to extend this understanding to higher dimensions. In previous works,\cite{Mandal:2015jla}\cite{Mandal:2015kxi}, we have seen that the post quench system equilibriates to a generalised Gibb's Ensemble. The post-quench observables retain a memory of the quench by having signatures set by the scale of the pre-quench state. We restrict our calculations to two kinds of pre-quench states: the ground state of the pre-quench Hamiltonian, and specific excited states called the squeezed states (CC and GCC). \par All observables seem to reach an equilibrium. The correlation functions in the CC approach a thermal ensemble and those in the GCC approach a GGE, at late times, and are related by, $\beta=4\kappa_2$ and $\mu=4\kappa_4$. We observe a distinction between odd and even dimensions. The approach to equilibrium is exponentially decaying in time for odd $d$ and fall off as a power law for even $d$. We also calculate the time dependent thermal correlator and observe a similar difference in odd and even dimensions. \par In the second last section, we discuss the possibility of UV-IR mixing in the GCC and GGE. The post-quench state is characterized by infinite number of conserved charges which may correspond to irrelevant operators in the theory. Observables seem to be affected by all such operators even at low energies, which is interesting given our intuitions set by Wilsonian renormalization. \par Finally, we wish to understand the implications of this result in the context of holography, with the knowledge that thermalization in the gauge theory corresponds to a quasi-normal decay to a black-hole. A quench itself can correspond to an excitation in the bulk. en_US
dc.language.iso en en_US
dc.subject 2018
dc.subject Physics en_US
dc.subject Quantum Quench en_US
dc.subject Holography en_US
dc.subject Two point functions en_US
dc.subject Thermalization en_US
dc.subject Calabrese-Cardy en_US
dc.subject Generalised Gibb's Ensemble en_US
dc.title Quantum Quench and Thermalization in Free Scalar Field Theory and its Gravity Dual (In Arbitrary Dimensions) en_US
dc.type Thesis en_US
dc.type.degree BS-MS en_US
dc.contributor.department Dept. of Physics en_US
dc.contributor.registration 20131010 en_US


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  • MS THESES [1705]
    Thesis submitted to IISER Pune in partial fulfilment of the requirements for the BS-MS Dual Degree Programme/MSc. Programme/MS-Exit Programme

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