

Starts With a Bang #96 - Detecting the Cosmic Gravitational Wave Background
Aug 12, 2023
Chapters
Transcript
Episode notes
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27
Introduction
00:00 • 2min
The New Type of Gravitational Wave Signals
01:48 • 4min
Einstein's Theory of Gravity
05:58 • 5min
The Origins of Gravitational Waves in the Universe
10:38 • 5min
How to Measure Space-Time Ripples With a Laser Interferometer
15:38 • 5min
The Difference Between Detecting the Background and Characterizing the Background
21:06 • 5min
The Future of Pulsar Observation
25:45 • 3min
The Future of Supermassive Black Hole Detection
28:35 • 5min
The Importance of Arrays in Radio Astrophysics
33:26 • 5min
The Effects of Air SIBO on Observation
37:56 • 5min
The Future of Pulsar Timing
43:03 • 6min
The Future of Pulsar Timing Arrays
48:59 • 2min
The Special Types of Pulsars
50:49 • 4min
The Glitch in the Universe
55:10 • 5min
Gravitational Wave Correlation Patterns
01:00:03 • 2min
The Future of Pulsars
01:02:16 • 5min
The Probability of Finding Neutron Stars on Voyager One
01:06:51 • 2min
The Most Massive Neutron Star Ever Discovered
01:08:40 • 2min
J0740 Plus 6620: A Millisecond Pulsar
01:10:45 • 2min
The Limits of Neutron Stars
01:13:14 • 4min
The Importance of Laboratory Experiments in Astronomy
01:17:29 • 6min
The Relationship Between Pressure and Density in Neutron Star Interiors
01:23:17 • 2min
The Importance of Precision in Pulsar Timing
01:25:16 • 4min
Pulsar Timing and Dark Matter
01:28:48 • 3min
The Future of Pulsar Timing
01:31:37 • 4min
The Nanograph Collaboration: A Student's Perspective
01:35:46 • 2min
The History of the Universe: One Page at a Time
01:37:35 • 4min