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Gravitational solitons and non-relativistic string theory

Published 17 Jan 2025 in hep-th | (2501.10178v2)

Abstract: We explore the non-relativistic string theory (NRST) limit of type II string theory and its action on gravitational solitons. As a start, we exhibit in detail that the NRST limit is T-dual to a discrete lightcone limit and can be viewed as a near-BPS limit. This also clarifies the nature of multi-string states of NRST and its connection to matrix string theory. We consider the NRST limit of the fundamental string soliton, confirming the recent finding that it corresponds to a relativistic near-horizon background, which we argue is the manifestation of a strong coupling phase of the NRST worldvolume theory. Furthermore, we consider the NRST limit of a class of D-branes as well as the NS5-brane. This reveals that they become gravitational solitons in NRST, as they are sourced torsional string Newton-Cartan (TSNC) geometries. Finally, for the NRST D-brane solitons we show that a further decoupling limit leads to new holographic correspondences between multicritical matrix theories and NRST in curved TSNC backgrounds.

Summary

  • The paper establishes the non-relativistic string theory (NRST) limit and its duality to discrete light cone quantization as a near-BPS regime.
  • It demonstrates how gravitational solitons, including fundamental strings and D-branes, emerge through torsional Newton-Cartan geometries.
  • The study uncovers novel holographic correspondences linking NRST to matrix string theories and multicritical models in curved TSNC backgrounds.

Overview of "Gravitational Solitons and Non-Relativistic String Theory"

The study presented in "Gravitational Solitons and Non-Relativistic String Theory" explores the non-relativistic string theory (NRST) by exploring its interplay with gravitational solitons arising within the context of type II string theory. The paper achieves a rigorous examination of the NRST limit, analyzing its dual nature with discrete light cone quantization (DLCQ) and its representation as a near-BPS limit. The research broadens the understanding of non-relativistic strings, linking them with matrix string theory and providing insights into potential new holographic correspondences.

Non-Relativistic String Theory (NRST) Limit

The authors initiate their investigation with a detailed exposition of the NRST limit. They illustrate its T-dual correspondence to a DLCQ as well as its interpretation as a near-BPS limit. This approach reveals substantial insights into the spectrum and dynamics of NRST, especially highlighting its strong coupling phase manifested in relativistic near-horizon backgrounds. The analysis extends to multi-string states, offering a comprehensive picture of interactions within NRST by establishing connections with matrix string theory.

Gravitational Solitons in NRST

The paper's pivotal exploration is into the gravitational solitons under the NRST limit, particularly focusing on fundamental strings and D-brane configurations. It is shown that the NRST limit of the fundamental string soliton corresponds to a relativistic near-horizon background due to the infinite backreaction in the strong coupling phase of the NRST worldsheet theory. This duality is further nuanced with the consideration of torsional string Newton-Cartan (TSNC) geometries, with transverse D-branes and NS5-branes becoming viable gravitational solitons in NRST.

Implications on Holographic Correspondences

The implications of these gravitational configurations stretch into the domain of holography. For instance, the NRST D-brane solitons uncovered in this research provide a pathway to new holographic correspondences through a decoupling limit. This limit elucidates correspondences between multicritical matrix theories and NRST within curved TSNC backgrounds. Such findings contribute saliently to understanding the holographic principle in contexts that deviate from Lorentzian symmetries.

Future Directions and Theoretical Implications

This paper not only fortifies the foundational aspect of NRST but also encourages further probing into holographic principles diverging from conventional forms. The exploration into non-relativistic limits bridges gaps between NRST and observables in holography and supersymmetric sectors in string theory. It opens a dialogue for examining quantum geometries and compactifications within broader frameworks of string theories, leveraging torsional Newton-Cartan structures.

Moreover, the study sets a foundation for further scrutiny of non-zero temperature backgrounds and understanding potential parallels to TTˉT\bar{T} deformations, enhancing both the breadth and depth of NRST applications in modern theoretical physics. The fidelity with which the paper navigates these complex interactions underscores the intricate tapestry of interactions in the string theory landscape.

In conclusion, this work provides a robust platform for advancing non-relativistic string theory, elucidating gravitational solitons, and expanding our conceptual framework of holographic dualities, presenting NRST as not only a mathematical construct but a physical reality with far-reaching implications and applications.

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