Starts With A Bang podcast

Starts With a Bang #96 - Detecting the Cosmic Gravitational Wave Background

Aug 12, 2023
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1
Introduction
00:00 • 2min
2
The New Type of Gravitational Wave Signals
01:48 • 4min
3
Einstein's Theory of Gravity
05:58 • 5min
4
The Origins of Gravitational Waves in the Universe
10:38 • 5min
5
How to Measure Space-Time Ripples With a Laser Interferometer
15:38 • 5min
6
The Difference Between Detecting the Background and Characterizing the Background
21:06 • 5min
7
The Future of Pulsar Observation
25:45 • 3min
8
The Future of Supermassive Black Hole Detection
28:35 • 5min
9
The Importance of Arrays in Radio Astrophysics
33:26 • 5min
10
The Effects of Air SIBO on Observation
37:56 • 5min
11
The Future of Pulsar Timing
43:03 • 6min
12
The Future of Pulsar Timing Arrays
48:59 • 2min
13
The Special Types of Pulsars
50:49 • 4min
14
The Glitch in the Universe
55:10 • 5min
15
Gravitational Wave Correlation Patterns
01:00:03 • 2min
16
The Future of Pulsars
01:02:16 • 5min
17
The Probability of Finding Neutron Stars on Voyager One
01:06:51 • 2min
18
The Most Massive Neutron Star Ever Discovered
01:08:40 • 2min
19
J0740 Plus 6620: A Millisecond Pulsar
01:10:45 • 2min
20
The Limits of Neutron Stars
01:13:14 • 4min
21
The Importance of Laboratory Experiments in Astronomy
01:17:29 • 6min
22
The Relationship Between Pressure and Density in Neutron Star Interiors
01:23:17 • 2min
23
The Importance of Precision in Pulsar Timing
01:25:16 • 4min
24
Pulsar Timing and Dark Matter
01:28:48 • 3min
25
The Future of Pulsar Timing
01:31:37 • 4min
26
The Nanograph Collaboration: A Student's Perspective
01:35:46 • 2min
27
The History of the Universe: One Page at a Time
01:37:35 • 4min