Search for spinning black hole binaries in advanced ligo parameter tuning of hacr
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Search for Spinning Black Hole Binaries in Advanced LIGO: Parameter tuning of HACR. Speaker: Gareth Jones Cardiff University LSC Meeting March 2005 ASIS session DCC#: G050201-00-Z. Overview. Goal: Detection of SBBH’s in Time Frequency representation of Advanced LIGO data What is HACR?

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Search for spinning black hole binaries in advanced ligo parameter tuning of hacr

Search for Spinning Black Hole Binaries in Advanced LIGO: Parameter tuning of HACR

Speaker: Gareth Jones

Cardiff University

LSC Meeting March 2005

ASIS session

DCC#: G050201-00-Z

Spinning Black Hole Binaries


Overview
Overview

Goal: Detection of SBBH’s in Time Frequency representation of Advanced LIGO data

  • What is HACR?

  • Spinning Black Hole Binaries

  • Tuning HACR in 2 steps

  • Results

  • Conclusions and Future Work

Spinning Black Hole Binaries


What is hacr
What is HACR?

  • Hierarchical Algorithm for Clusters and Ridges written by R. Balasubramanian

  • Time-frequency search

  • Short bursts of excess power

  • More robust than matched-filtering

  • Implemented in GEO++ as HACRMon

Spinning Black Hole Binaries


How hacr works
How HACR works

1. Identify pixels with P > ηupper

Frequency

Time

Spinning Black Hole Binaries


How hacr works1
How HACR works

1. Identify pixels with P > ηupper

“Black pixels”

Frequency

Time

Spinning Black Hole Binaries


How hacr works2
How HACR works

2. Identify neighbouring pixels with P > ηlower

“Black pixels”

Frequency

Time

Spinning Black Hole Binaries


How hacr works3
How HACR works

2. Identify neighbouring pixels with P > ηlower

“Cluster”

Frequency

Time

Spinning Black Hole Binaries


How hacr works4
How HACR works

3. Identify clusters with Npixels > Nthreshold

“Cluster”

Frequency

Time

Spinning Black Hole Binaries


How hacr works5
How HACR works

3. Identify clusters with Npixels > Nthreshold

“Event”

Frequency

Time

Spinning Black Hole Binaries


Spinning black hole binaries
Spinning Black Hole Binaries

  • Require 17 physical parameters to accurately describe waveform

  • Spin-induced precession of orbital plane causes modulation of amplitude and phase

  • Amplitude modulation causes of GW “archipelago” of clusters in TF map

Spinning Black Hole Binaries


Spinning black hole binaries1
Spinning Black Hole Binaries

Amplitude

Amplitude

Time

Time

Frequency

Frequency

Time

Time

Spinning Black Hole Binaries


Tuning hacr
Tuning HACR

For a given false alarm rate maximise

probability of detection

  • Identify combinations of threshold parameters (ηupper,Nthreshold ) that produce a constant false alarm rate…

  • … then for each combination of parameters measure probability of detection

Spinning Black Hole Binaries


False alarm analysis
False Alarm Analysis

  • 100,000s of simulated Adv. LIGO data

  • Analyse with low values of ηupper and Nthreshold

  • Store maximum-power and number of pixels for each found “event”

  • For range of ηupper choose values of Nthreshold that give specific False Alarm rates

Spinning Black Hole Binaries


False alarm analysis1
False Alarm Analysis

Contours of constant false alarm rate

1 False alarm per…

Nthreshold

…hour (27.8 events)

…1000s (100 events)

…10 mins (166.7 events )

…100s (1000 events)

…min (1666.7 events)

…10s (10,000 events)

ηupper

Spinning Black Hole Binaries


Injection of sbbh waveforms
Injection of SBBH waveforms

  • Physical waveforms

  • (1-49), (10-40) and (25-25)Msolar

  • 1000 injections each with SNR = 8,12,16

  • Measure number of injections recovered for each combination of (ηupper,Nthreshold )

Spinning Black Hole Binaries


Results
Results

SNR = 16

# of recovered injections

SNR = 12

SNR = 8

Expected # of FA = ~54

ηupper

Spinning Black Hole Binaries


Results1
Results

Small spin modulation

Large spin modulation

(1-49)M

(1-49)M

(10-40)M

(10-40)M

(25-25)M

(25-25)M

Spinning Black Hole Binaries


Results2
Results

Small spin modulation

Large spin modulation

(1-49)M

(1-49)M

(10-40)M

(10-40)M

(25-25)M

(25-25)M

ηupper = 23, Nthreshold = 50

Spinning Black Hole Binaries


Conclusion and future work
Conclusion and Future Work

  • More injections and at various distances

  • Power law pattern matching for potential event clusters

  • Tune HACR for EMRI signals in LISA (with Jonathan Gair)

Spinning Black Hole Binaries


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