Presentation is loading. Please wait.

Presentation is loading. Please wait.

Matched Filtering Junwei Cao (曹军威) and Junwei Li (李俊伟)

Similar presentations


Presentation on theme: "Matched Filtering Junwei Cao (曹军威) and Junwei Li (李俊伟)"— Presentation transcript:

1 Matched Filtering Junwei Cao (曹军威) and Junwei Li (李俊伟)
Tsinghua University Gravitational Wave Summer School Kunming, China, July 2009 1

2 Weak Signals, Loud Noise
In Signals are weak How to dig out GW signals If we know, at least to some level of accuracy, the form of h(t)

3 A Sample Filtering Multiply s(t) by h(t)

4 A Sample Filtering (contd.)
T can’t be infinite Not necessary to have h0>n0 For example, τ0=1 ms, T=1 year

5 Optimal Filtering To obtain the highest possible SNR Define
SNR definition (in amplitude) : Filter function

6 S & N

7 S/N Using eq. 1.7 Therefore

8 What is the Filter K(t) Define a scalar product Then

9 The Solution Search for the “vector” unit norm
So, the matched filter is

10 The Optimal Value of SNR
Insert eq into 2.11 Insert ea into 2.10

11 Bursts What are bursts? From astrophysical phenomena, e.g. supernova explosions, final merging of a neutron star-neutron star binary system Large energy, short time, typically less than a second Hard to know the form of Use order-of-magnitude estimate 11

12 Narrow-band Detectors
Only sensitive to frequencies in a bandwidth , centered around cannot change much Approximate with Eq becomes 12

13 Broad-band Detectors Bandwidth Order-of-magnitude estimate
: characteristic value of over : characteristic value of over A detailed form of bursts is important 13

14 A Model for Bursts A sine-Gaussian : the amplitude : the duration
Fourier transform If , near , basically Gaussian Maximum of the Gaussian: 14

15 Estimate Minimum h0 When ,  relatively flat
When ,  sharply peaked around For narrow-band detectors, plug eq into eq. 2.16 For broad-band detectors, plug eq into eq. 2.17 15

16 Root-sum-square Amplitude
defined by For sine-Gaussian 16

17 An Exercise The total energy radiated by the source in GWs, assuming a sine-Gaussian waveform A sine-Gaussian burst (1ms duration, 1kHz ) which release 1/100 solar masses in the Virgo galaxy cluster, which is at r~14Mpc Requirement Approximate and 17

18 Answer

19 Thank You ! Junwei Cao 19


Download ppt "Matched Filtering Junwei Cao (曹军威) and Junwei Li (李俊伟)"

Similar presentations


Ads by Google