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1
Introduction
2
What are neutronstars
3
Orbital dynamics
4
Gravitationalwave
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Oversimplified picture
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Deformations
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Waveform models
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Universal relations
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Equivalent waveforms
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Descriptive bottleneck
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Properties of matter
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Functional forms
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Gravitationalwave data
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Other observations
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Representational challenges
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Model comparison
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Terrestrial experiments
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Nuclear theory
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Comparing observations
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Future generation observatories
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Other ways
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Galactic neutronstars
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New mass distribution
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Missing something important
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Next generation
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Communication
Description:
Explore the latest discoveries in gravitational-wave astronomy and their implications for understanding neutron stars and dense matter in this 41-minute lecture by Jocelyn Read from California State University, Fullerton. Delve into the groundbreaking observations made by LIGO, Virgo, and KAGRA, including the neutron-star/black-hole mergers GW200105 and GW20011, and the heavy neutron-star merger GW190425. Learn about methods used to investigate matter and mass properties of LIGO/Virgo neutron stars, and how these findings align with other neutron-star observations. Gain insights into the potential of current Advanced-detector era and future next-generation gravitational-wave observatories like Cosmic Explorer in mapping the phase diagram of dense neutron-rich matter and revealing the endpoints of stellar evolution. Discover how the distribution of masses in compact binary mergers is becoming a crucial observable in gravitational-wave astronomy and its implications for our understanding of the universe. Read more

Gravitational-Wave Observations of Neutron-Star Mergers - IPAM at UCLA

Institute for Pure & Applied Mathematics (IPAM)
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