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Time Delay Cosmography: A New Lens on the Hubble Tension

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Manage episode 515399732 series 3690682
Content provided by Mike Breault. All podcast content including episodes, graphics, and podcast descriptions are uploaded and provided directly by Mike Breault or their podcast platform partner. If you believe someone is using your copyrighted work without your permission, you can follow the process outlined here https://podcastplayer.com/legal.
Brought to you by embersilk.com. A deep dive into how strong gravitational lensing time delays offer an independent route to measuring the Hubble constant. We'll unpack the mass-sheet degeneracy, the role of stellar kinematics and line-of-sight mass, and the latest results from the TDCOSMO collaboration. Simple lens models tend to yield H0 around 73 km/s/Mpc, aligned with local measurements, while more flexible, kinematics-informed models pull H0 toward the Planck value but with larger uncertainties. We discuss what this means for lambda cold dark matter cosmology and whether resolving the tension might point to new physics—or simply demand better modeling and more data.

Note: This podcast was AI-generated, and sometimes AI can make mistakes. Please double-check any critical information.

Sponsored by Embersilk LLC

  continue reading

1404 episodes

Artwork
iconShare
 
Manage episode 515399732 series 3690682
Content provided by Mike Breault. All podcast content including episodes, graphics, and podcast descriptions are uploaded and provided directly by Mike Breault or their podcast platform partner. If you believe someone is using your copyrighted work without your permission, you can follow the process outlined here https://podcastplayer.com/legal.
Brought to you by embersilk.com. A deep dive into how strong gravitational lensing time delays offer an independent route to measuring the Hubble constant. We'll unpack the mass-sheet degeneracy, the role of stellar kinematics and line-of-sight mass, and the latest results from the TDCOSMO collaboration. Simple lens models tend to yield H0 around 73 km/s/Mpc, aligned with local measurements, while more flexible, kinematics-informed models pull H0 toward the Planck value but with larger uncertainties. We discuss what this means for lambda cold dark matter cosmology and whether resolving the tension might point to new physics—or simply demand better modeling and more data.

Note: This podcast was AI-generated, and sometimes AI can make mistakes. Please double-check any critical information.

Sponsored by Embersilk LLC

  continue reading

1404 episodes

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