Accretion, mergers, and metastability of fuzzy spheres in a three-matrix model
Abstract
A three-matrix model that contains a plethora of fuzzy sphere solutions was defined twenty years ago. It has been shown that in a certain regime of the model, combinations of fuzzy spheres become classical solutions of the model. In the original paper and subsequent works, the stability of specific states has been discussed, showing that only a single largest fuzzy-sphere configuration is stable. Here, we focus on a complementary question: starting from some initial configuration, is the thermodynamically preferred state approached rapidly, or are there other long-lived, metastable configurations which may support interesting physics? We find that the answer in the large-matrix limit depends on the dispersion of the initial configuration. We identify the elementary transition as an accretion, in which one sphere absorbs a single unit from another, and show that it is driven by fluctuations of the sphere centers. By measuring these fluctuations in long simulations, we find quantitative agreement with the one-loop effective action, with no free parameters. For multi-sphere states, we find that the stiffness of an inner sphere grows logarithmically with the number of surrounding layers, so that concentric onion-like configurations -- describing an emergent three-dimensional quantum space -- become increasingly long-lived.
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BibTeX
@misc{hrmo2026accretion,
title = {{Accretion, mergers, and metastability of fuzzy spheres in a three-matrix model}},
author = {M. Hrmo and S. Kováčik and K. Magdolenová and A. Manta and K. Nedeľková and P. Rusnák and H. C. Steinacker and J. Tekel},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.00328},
eprint = {2609.00328},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.00328},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Accretion, mergers, and metastability of fuzzy spheres in a three-matrix model
AU - M. Hrmo
AU - S. Kováčik
AU - K. Magdolenová
AU - A. Manta
AU - K. Nedeľková
AU - P. Rusnák
AU - H. C. Steinacker
AU - J. Tekel
PY - 2026
DA - 2026/09/01
PB - arXiv
DO - 10.48550/arxiv.2609.00328
UR - https://arxiv.org/abs/2609.00328
AB - A three-matrix model that contains a plethora of fuzzy sphere solutions was defined twenty years ago. It has been shown that in a certain regime of the model, combinations of fuzzy spheres become classical solutions of the model. In the original paper and subsequent works, the stability of specific states has been discussed, showing that only a single largest fuzzy-sphere configuration is stable. Here, we focus on a complementary question: starting from some initial configuration, is the thermodynamically preferred state approached rapidly, or are there other long-lived, metastable configurations which may support interesting physics? We find that the answer in the large-matrix limit depends on the dispersion of the initial configuration. We identify the elementary transition as an accretion, in which one sphere absorbs a single unit from another, and show that it is driven by fluctuations of the sphere centers. By measuring these fluctuations in long simulations, we find quantitative agreement with the one-loop effective action, with no free parameters. For multi-sphere states, we find that the stiffness of an inner sphere grows logarithmically with the number of surrounding layers, so that concentric onion-like configurations -- describing an emergent three-dimensional quantum space -- become increasingly long-lived.
ER -