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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

  • FRB AND SCATTERING
  • TWO SCREEN MODELLING
  • RESOLUTION ARGUMENT
  • ACF AND MODULATION INDEX
  • QUENCHING OF SCINTILLATIONS!
  • SUMMARY

Multi Screen FRB

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FAST RADIO BURSTS

  • Fast Radio Bursts (FRBs) are extra-galactic single pulses of micro to millisecond duration.
  • Encounters Host galaxy ISM, Intergalactic Medium, Milkyway ISM.
  • Propagation effects: Dispersion, Rotation Measure, Scattering and Scintillation.
  • FRBs as an astrophysical tool. 

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FRB 20220207C (Zach) detected by DSA , MB. Sherman et al.2023

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Multi Screen FRB

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SCATTERING AND SCINTILLATION

Multi Screen FRB

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  • Multipath propagation of pulse causes delayed arrivals.
  • Pulse Broadening due to scattering.
  • Delays (τ) shorter than pulse duration interferes to produce scintillations of bandwidth 1/τ in frequency space . 
  • Scattering material approximated to be distributed in thin screens/lens

Courtesy - Dr. Robert Main

Scatter Tail

Interference

pattern

FRB

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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

  • Fourier uncertainty,  2πtscatter𝜈scint =1
  • Violated by a number of FRBs (eg: Sammons et al. 2023)
  • Major pulse scattering : Host galaxy screen.
  • Scintillation effects : Milky Way (MW) screen.

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TWO SCREEN MODELLING

Multi Screen FRB

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  • Total geometric delay  due to a path of multiple deflection is the sum of delay due to each deflection from straight line. Time delay from screenj and screeni,
  • Image distribution: Random, overlayed with gaussian amplitude distribution.

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  • Stars twinkle, planets don’t.
  • What happens when host galaxy screen is resolved? Will it be like resolving a planet?
  • Presence of MW scintillation used to put limits on location of host galaxy screen (Masui et al. 2015)
  • Resolution Power, RP = θhost/θres  

RP > 1 : Resolved

    RP < 1 : Unresolved

Multi Screen FRB

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Unresolved

Resolved

RESOLVING SCREENS IN FRBS

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SPECTRAL ACF AND MODULATION INDEX

  • The two screen delay formula can written as:

Multi Screen FRB

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  • FFT of the time series into the spectra. The spectral ACF in the two screen unresolved regime becomes
  • N-Screen ACF and modulation index:

&

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Multi Screen FRB

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NOW SIMULATIONS👉🏾

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ABRUPT QUENCHING OF SCINTILLATION?

Multi Screen FRB

Multi Screen FRB

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Just Resolved

Un-Resolved Screens

More Resolved

Completely Resolved screens

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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!

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  • Broad Scintillation – MW Screen
  • mMW 1
  • 𝜈MW,simulation = 𝜈MW,injected

Multi Screen FRB

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SPECTRAL ACF – RP=0

  • Narrow Scintillation – Host screen
  • Total two screen modulation, mtot √3
  • 𝜈host,simulation = 𝜈host,injected

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  • mMW < 1
  • 𝜈MW,simulation > 𝜈MW,injected

Multi Screen FRB

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SPECTRAL ACF – RP= 1

  • Total two screen modulation, mtot < √3
  • 𝜈host,simulation = 𝜈host,injected

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  • mMW < 1
  • 𝜈MW,simulation >> 𝜈MW,injected

Multi Screen FRB

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SPECTRAL ACF – RP = 10

  • Total two screen modulation, mtot 1
  • 𝜈host,simulation = 𝜈host,injected

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INTRA-PULSE SCINTILLATION EVOLUTION

Spectrum (t)

ACF of each Spectrum (t)

Coherence length decreasing along the scattering tail

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Multi Screen FRB

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 INTRA-PULSE MODULATION EVOLUTION

 Case-1: Unresolved Screens 

 Case-3: Resolving Screens 

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Multi Screen FRB

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APPLICATION OF QUENCHING

  • Broadening and quenching of scintillation with increase in RP.
  • Peak ACF value (ACFMW) of the MW Scintillation fit gives an upper limit on the host galaxy screen distance from the host.

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

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Multi Screen FRB

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PREDICTION - BROADBAND STUDIES!

  • Following θbroadening ∝ 𝜈-2 ; RP ∝ 𝜈-3  for a two screen system.
  • A broadband pulse could show the transition from unresolved screens to resolved screens. (Tim's talk!) 

2-Resolving Screens

Screen resolving incoherent emission region

  • Screen resolves the emission region – Scintillation is quenched. Constant emission region size, RP ∝ 𝜈-1.
  • Observations: Nimmo et al 2024, observes this in FRB 20221022A. 

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Multi Screen FRB

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SUMMARY AND FUTURE

  • Multi-Screen Scattering Model: Incorporating cosmology for a general model for multi-screen scattering. 
  • Scintillation Quenching in Two-Screen Systems: Evidence for gradual diminishing broad scintillation with increased resolution in two-screen systems.
  • Host Screen Distance: New formula to position screens and proved through simulations. Caveat – does not work for 1-D screens.
  • Broadband studies: Two resolving screens or screen resolve emission regions of FRBs/Pulsars have observable trends in 𝜈scint ∝ 𝜈a
  • MW Screens: For two 1 AU screens at a separation of 1 kpc, RP = 750?!? -- means only one scale of scintillation survives.

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THANK YOU!

ACKNOWLEDGEMENTS

  • DR. TIM SPRENGER
  • DR. OLAF WUCKNITZ
  • DR. ROBERT MAIN
  • DR. LAURA SPITLER

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FRB-SCINTILATOR – TWO SCREEN

  • Starting from an image distribution over laid with a gaussian intensity distribution
  • Total multi-screen effect: 

HOST GALAXY SCREEN

MILKY WAY SCREEN

  • Each pair of image points comprise a path of propagation

Multi Screen FRB

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Each path has an amplitude and phase

Ai . Aj

AMW

Ahost

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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!

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Multi Screen FRB

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1-D SCREENS

 Case-1: 1-D parallel screens 

 Case-1: 1-D perpendicular screens 

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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

  • Distance limit formula:
  • Comparison of distance limit 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