University of Cambridge > Talks.cam > Cosmology Lunch > Cosmological Perturbation Theory

  Browse A-Z

Log in

University Account External (via Google)

🔐 Log In

Information on

Subscribing to talksdetails Finding a talkdetails Adding a talkdetails Disseminating talksdetails Help and Documentationdetails

ℹī¸ Information

Cosmological Perturbation Theory

Download to your calendar using vCal

If you have a question about this talk, please contact David Stefanyszyn .

Cosmological perturbation theory is an important theoretical pillar in the development and success of modern cosmology. Using the ADM (3+1) formulation of Einstein’s gravity a perturbation analysis valid to fully nonlinear and exact order is possible. Being fully nonlinear and exact it includes any order perturbation expansion as well as the post-Newtonian approximation. We will explain some consequences of this formulation in cosmology and astrophysics. A related work we have devoted during our stay in DAMTP will be explained as well.

This talk is part of the Cosmology Lunch series.

This talk is included in these lists:

Note that ex-directory lists are not shown.

Other lists

Average on weekdays: 9039.34259259 kWh Library of Cambridge Union Society CB2 1UB RCM London,Outer Parry Room

Other talks

Title to be confirmed Title to be confirmed Title to be confirmed Christopher Cowie on the epistemology of assessing biosignature claims Title to be confirmed TBC
 

Š 2006-2025 Talks.cam, University of Cambridge. Contact Us | Help and Documentation | Privacy and Publicity