Baby universes and energy (non-)conservation in (1+1)-dimensional dilaton gravity
V.A. Rubakov

TL;DR
This paper studies baby universe branching in (1+1)-dimensional dilaton gravity, revealing that energy is not conserved during baby universe emission, with implications for locality and long-range fields.
Contribution
It demonstrates non-conservation of energy in baby universe processes within (1+1)-dimensional dilaton gravity and proposes a scenario involving long-range dilaton fields and gravitational waves.
Findings
Energy non-conservation due to baby universe emission
Finite probability of baby universe branching with local matter
Long-range dilaton fields may reconcile non-conservation with locality
Abstract
We consider branching of baby universes off parent one in (1+1)-dimensional dilaton gravity with 24 types of conformal matter fields. This theory is equivalent to string theory in a certain background in D=26-dimensional target space, so this process may be also viewed as the emission of a light string state by a heavy string. We find that bare energy is not conserved in (1+1) dimensions due to the emission of baby universes, and that the probability of this process is finite even for local distribution of matter in the parent universe. We present a scenario suggesting that the non-conservation of bare energy may be consistent with the locality of the baby universe emission process in (1+1) dimensions and the existence of the long ranged dilaton field whose source is bare energy. This scenario involves the generation of longitudinal gravitational waves in the parent universe.
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