PIRSA:18060007

Dicke’s Superradiance -- From millisecond fast radio bursts (FRBs) to multiyear maser bursts

Rajabi, F. (2018). Dicke’s Superradiance -- From millisecond fast radio bursts (FRBs) to multiyear maser bursts. Perimeter Institute. https://pirsa.org/18060007

Rajabi, Fereshteh. Dicke’s Superradiance -- From millisecond fast radio bursts (FRBs) to multiyear maser bursts. Perimeter Institute, Jun. 26, 2018, https://pirsa.org/18060007 

          @misc{ pirsa_PIRSA:18060007,
            doi = {10.48660/18060007},
            url = {https://pirsa.org/18060007},
            author = {Rajabi, Fereshteh},
            keywords = {Cosmology},
            language = {en},
            title = {Dicke{\textquoteright}s Superradiance -- From millisecond fast radio bursts (FRBs) to multiyear maser bursts},
            publisher = {Perimeter Institute},
            year = {2018},
            month = {jun},
            note = {PIRSA:18060007 see, \url{https://pirsa.org}}
          }

Fereshteh Rajabi

McMaster University

Talk number
PIRSA:18060007
Collection
Talk Type
Subject
Abstract

Burst phenomena are ubiquitous in astrophysics. Understanding the origin of bright and rapid bursts, like FRBs, is an important goal of contemporary astrophysics.  We apply Dicke's superradiance, a coherent quantum mechanical radiation mechanism, to explain these burst phenomena. We show that bursts lasting from a few milliseconds (FRBs) to a few years (e.g. OH masers) can be produced by very large groups of entangled atoms/molecules. This is in contrast with the common assumption that, in the interstellar medium, the atoms/molecules in a radiating gas act independently from each other. Superradiance, a well-known and intensely studied phenomenon in the physics community, was first discussed by R. H. Dicke in 1954. I will present our superradiance models developed to explain some maser flares and FRBs, and discuss our results for the 6.7-GHz methanol, 1612-MHz OH, and 22-GHz water spectral lines. Our analyses suggest that the aforementioned groups of entangled atoms/molecules, developing over distances of up to a few kilometers for maser flares and 1000 AU for FRBs, can reproduce the observed light curves