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on
1
Introduction
2
Application to cosmology
3
Tensions between different experiments
4
Center siren method
5
Electromagnetic counterpart
6
Projections
7
Next generation detector
8
Single galaxy localization
9
Dark siren approach
10
Can we do better
11
What is this degeneracy
12
Break this degeneracy
13
Measuring the distance
14
EM observations
15
Selection effect
16
Calibration uncertainty
17
Miscalibration
18
Summary
19
Questions
20
Plot
21
Redshift
22
Binary neutron star rate
23
Other questions
24
Crosscorrelation
25
Results
Description:
Explore gravitational-wave standard sirens with electromagnetic counterparts in this 44-minute lecture by Hsin Yu Chen from MIT. Delve into the groundbreaking field of gravitational wave detection and its impact on physics, stellar evolution, and cosmology. Learn about the application of standard sirens to cosmology, tensions between different experiments, and the center siren method. Discover electromagnetic counterparts, projections for next-generation detectors, and single galaxy localization techniques. Examine the dark siren approach, methods to break degeneracies, and the challenges of measuring distances. Investigate electromagnetic observations, selection effects, and calibration uncertainties. Gain insights into binary neutron star rates, crosscorrelation techniques, and the latest results in this cutting-edge area of astrophysics.

Gravitational-Wave Standard Sirens With Electromagnetic Counterparts - Hsin Yu Chen

Kavli Institute for Theoretical Physics
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