Search for the most stable massive state in superstring theory
Diego Chialva, Roberto Iengo, Jorge G. Russo

TL;DR
This paper investigates the stability and decay properties of massive states in superstring theory, identifying the most stable configurations and their lifetimes, with implications for understanding string decay channels and spectra.
Contribution
It introduces the concept of a highly stable rotating ring state in superstring theory and quantifies its lifetime and decay channels, a novel insight into string stability.
Findings
The average string state lifetime scales as 1/(g^2 M).
The most stable state, the rotating ring, has a lifetime proportional to M^5/g^2.
Decay spectra of rotating rings resemble thermal spectra with a maximum and exponential tail.
Abstract
In ten dimensional type II superstring, all perturbative massive states are unstable, typically with a short lifetime compared to the string scale. We find that the lifetime of the average string state of mass M has the asymptotic form T < const.1/(g^2 M). The most stable string state seems to be a certain state with high angular momentum which can be classically viewed as a circular string rotating in several planes ("the rotating ring"), predominantly decaying by radiating soft massless NS-NS particles, with a lifetime T = c_0 M^5/g^2. Remarkably, the dominant channel is the decay into a similar rotating ring state of smaller mass. The total lifetime to shrink to zero size is ~ M^7. In the presence of D branes, decay channels involving open strings in the final state are exponentially suppressed, so the lifetime is still proportional to M^5, except for a D brane at a special angle or…
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.
