Introduction to Primordial Black Hole Dark Matter - Lecture 2
Offered By: International Centre for Theoretical Sciences via YouTube
Course Description
Overview
Syllabus
12:00 pm, 09 NOVEMBER 2020
Outline
Indirect detection: GWs from PBH Binary Mergers
Q: Does PBH Dark Matter have testable GW predictions?
Indirect Detection: The GW Mass Spectrum
Indirect Detection: Stellar Mass Spectrum
Indirect Detection: Constraints on PBH fraction
Indirect Detection: Orbital Eccentricity
Indirect Detection: Individual and Effective Spin
Indirect Detection: Stochastic GW Background
Indirect Detection: Clustering of GW Events
Indirect Detection: 03a Data Hot Off the Press!
Indirect Detection: 03a Fit with Astro Channels
Indirect Detection: 03a Fit with Accrediting PBHs
PBH Dark Matter: Constraining the Mass Fraction
Microlensing: Illustration
PBH Dark Matter: Existing Constraints
PBH Dark Matter: The "LIGO Window"
Direct Detection: New Transient Probes
Fast Radio Bursts!
Constraining MACHOs: Fast Radio Burst Lensing
Strong Lensing of FRBs: Unique Signature
PBH DM LIGO Window: Constraints Tightening!
Observational Outlook: Timeline
PBH DM: Other Windows Open?
From PBH to Primordial Power Spectrum Limits
PBHs as SMBH Seeds: Future Tight! Constraints
Takeaway: Lots of Ways to Probe PBH Scenario!
Thank you!
PBH DM: Other Windows Open?
Taught by
International Centre for Theoretical Sciences
Related Courses
Galaxies and CosmologyCalifornia Institute of Technology via Coursera From the Big Bang to Dark Energy
University of Tokyo via Coursera Astronomy - State of the Art
University of Arizona via Udemy Dark Matter in Galaxies: The Last Mystery
iversity Philosophy and the Sciences: Introduction to the Philosophy of Physical Sciences
University of Edinburgh via Coursera