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
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