TWO SCREEN SCINTILLOMETRY OF FRBS
SACHIN PRADEEP
LISE MEITNER GROUP ON FRB'S, FUNDAMENTAL PHYSICS IN RADIO ASTRONOMY, MPIFR - BONN
Lise Meitner Max Planck Research Group, Max-Planck-Institut für Radioastronomie
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AGENDA
Multi Screen FRB
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FAST RADIO BURSTS
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FRB 20220207C (Zach) detected by DSA , MB. Sherman et al.2023
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Multi Screen FRB
SCATTERING AND SCINTILLATION
Multi Screen FRB
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Courtesy - Dr. Robert Main
Scatter Tail
Interference
pattern
FRB
SCATTERING OBSERVABLES-SINGLE BURST
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Modulation index
mI - ACF Relation
Multi Screen FRB
tscatter, host
Screen Parameters
Measure of screen modulation in pulse spectra. In a single screen case its 1,
mI = STD(𝜈)/ MEAN(𝜈)
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Sammons et al. 2023
𝜈scint, MW
TWO SCREEN MODELLING
Multi Screen FRB
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RP > 1 : Resolved
RP < 1 : Unresolved
Multi Screen FRB
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7
Unresolved
Resolved
RESOLVING SCREENS IN FRBS
SPECTRAL ACF AND MODULATION INDEX
Multi Screen FRB
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&
Multi Screen FRB
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NOW SIMULATIONS👉🏾
ABRUPT QUENCHING OF SCINTILLATION?
Multi Screen FRB
Multi Screen FRB
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Just Resolved
Un-Resolved Screens
More Resolved
Completely Resolved screens
Multi Screen FRB
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DYNAMIC SPECTRA
Varying scintillation pattern!
Just Resolving
(RP=1)
Completely Resolved (RP=10)
Un-Resolving Screens (RP=0)
Varying scintillation pattern!
Multi Screen FRB
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SPECTRAL ACF – RP=0
Multi Screen FRB
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SPECTRAL ACF – RP= 1
Multi Screen FRB
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SPECTRAL ACF – RP = 10
INTRA-PULSE SCINTILLATION EVOLUTION
Spectrum (t)
ACF of each Spectrum (t)
Coherence length decreasing along the scattering tail
Multi Screen FRB
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INTRA-PULSE MODULATION EVOLUTION
Case-1: Unresolved Screens
Case-3: Resolving Screens
Multi Screen FRB
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APPLICATION OF QUENCHING
PROBING HOST GALAXY!
LFRB,h – Distance between source and host screen
LMW – Distance to MW screen
𝜈scint,MW - MW scintillation bandwidth
Tscatt,h – scattering time due to host screen
DFRB – Distance to FRB
Theoretically
Calculated Scint BW = 0.038MHz
Multi Screen FRB
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PREDICTION - BROADBAND STUDIES!
2-Resolving Screens
Screen resolving incoherent emission region
Multi Screen FRB
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SUMMARY AND FUTURE
THANK YOU!
ACKNOWLEDGEMENTS
FRB-SCINTILATOR – TWO SCREEN
HOST GALAXY SCREEN
MILKY WAY SCREEN
Multi Screen FRB
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Each path has an amplitude and phase
Ai . Aj
AMW
Ahost
Multi Screen FRB
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LOCATING HOST GALAXY SCREEN
The formulas proposed in literature so far to put an upper limit on host screen distance from FRB
Top: 2 Screen systems of different resolving power. Error bars through itterative cacluations of observables at different pulse widths.
New Formula GOOD!
Multi Screen FRB
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1-D SCREENS
Case-1: 1-D parallel screens
Case-1: 1-D perpendicular screens
Multi Screen FRB
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1-D SCREENS
Case-1: 1-D parallel screens
Case-1: 1-D perpendicular screens
Caveat for distance formula
True value : 5 kpc
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INTERPRETATION - PHYSICS BEHIND!
FRB
Host galaxy screen
Milky Way screen
Larger delay
Smaller delay, Larger scintillation