Non equivalence of Carroll limits in relativistic string theory
Roberto Casalbuoni, Daniele Dominici, Joaquim Gomis

TL;DR
This paper explores how Carroll limits of relativistic string theories lead to non-equivalent string models with different degrees of freedom, highlighting the effects of singular variable redefinitions.
Contribution
It demonstrates that Carroll limits can produce non-equivalent string theories with distinct degrees of freedom, due to singular transformations affecting configuration space and Lagrangians.
Findings
Carroll strings differ from their relativistic counterparts in degrees of freedom.
Singular redefinitions cause non-equivalence of theories after Carroll limit.
Different Carroll strings emerge depending on the initial relativistic theory.
Abstract
We construct new Carroll strings in flat space by considering the Carroll limit of equivalent relativistic string theories at classical level. In the limit these Carroll strings are no longer equivalent and have different degrees of freedom. This fact is due to a general phenomenon that the configuration space and canonical Lagrangians are no longer equivalent after a singular redefinition of the variables and of the parameters of the starting Lagrangians.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Relativity and Gravitational Theory
