Spacetime Energy Decreases under World-sheet RG Flow
Michael Gutperle, Matthew Headrick, Shiraz Minwalla, Volker, Schomerus

TL;DR
This paper demonstrates that in certain two-dimensional sigma models, the spacetime energy decreases along the renormalization group flow, aligning with known energy decrease phenomena in tachyon condensation.
Contribution
It establishes a connection between world-sheet RG flow and spacetime energy decrease using the Zamolodchikov c-theorem in asymptotically flat target spaces.
Findings
Spacetime energy decreases from UV to IR fixed points.
The result parallels energy decrease in tachyon condensation.
Uses the c-theorem to relate RG flow to energy changes.
Abstract
We study renormalization group flows in unitary two dimensional sigma models with asymptotically flat target spaces. Applying an infrared cutoff to the target space, we use the Zamolodchikov c-theorem to demonstrate that the target space ADM energy of the UV fixed point is greater than that of the IR fixed point: spacetime energy decreases under world-sheet RG flow. This result mirrors the well understood decrease of spacetime Bondi energy in the time evolution process of tachyon condensation.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
