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Schwinger Pair Production at Finite Temperature and Novel Astrophysical Probes of Millicharged Fermions

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dc.contributor.advisor THALAPILLIL, ARUN M. en_US
dc.contributor.author KORWAR, MRUNAL PRASHANT en_US
dc.date.accessioned 2018-05-10T03:17:30Z
dc.date.available 2018-05-10T03:17:30Z
dc.date.issued 2018-05 en_US
dc.identifier.uri http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/940
dc.description MS Thesis, 83 pages, 6 figures, final draft submitted to IISER Pune en_US
dc.description.abstract Schwinger pair production is a non-perturbative and non-linear phenomenon in Quantum Electrodynamics. It is equally interesting to theoretical and experimental physics because of the necessity of strong electric field required to study it. Many theoretical models have been developed to explain and extend the result for the number of pair produced from Scalar QED and QED vacuum. We use Worldline Instanton method to find vacuum decay rate for scalar QED and QED vacuum in presence of constant Electric field and constant Electric field parallel to the Magnetic field at zero temperature in weak field approximation and weak coupling limit. We thus verify results obtained by other theoretical methods for these field configurations. We extend the result to finite temperature case i.e. we give an analytical expression for Scalar QED and QED vacuum decay rate in presence of constant Electric field and constant Electric field parallel to the magnetic field at some non-zero temperature in weak field approximation and weak coupling limit. Schwinger pair production of electron-positron pairs requires a constant electric field of the order of $10^{18}V/m$. This huge electric field is not achieved in laboratory till now. Some of the astronomical objects like Magnetars do produce an electric field of the order of $10^{14}V/m$. Many extensions of the standard model generically give rise to hypothetical Millicharged particles. These are particles with fractional electric charges. Millicharged particles are interesting from the viewpoint of charge quantization and they are viable dark matter candidate too. Schwinger pair production of the Millicharged particle is possible in the Magnetar environment and affect the magnetic field evolution of magnetar. We provide a novel, model-independent constraints on these hypothetical particles based on Energy loss argument and Magnetic field evolution argument. We also show the effect of millicharged particles on the braking index of the magnetar. en_US
dc.description.sponsorship IISER Pune en_US
dc.language.iso en en_US
dc.subject 2018
dc.subject Physics en_US
dc.subject Natural Sciences en_US
dc.subject Quantum Electrodynamics en_US
dc.subject Scalar QED en_US
dc.subject Schwinger Pair Production en_US
dc.subject Novel Astrophysical Probes en_US
dc.subject Millicharged Fermions en_US
dc.title Schwinger Pair Production at Finite Temperature and Novel Astrophysical Probes of Millicharged Fermions 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 20131021 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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