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Non-Relativistic Gravity and its Coupling to Matter

4 Pith papers cite this work. Polarity classification is still indexing.

4 Pith papers citing it

citation-role summary

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citation-polarity summary

fields

gr-qc 2 hep-th 2

years

2026 4

roles

background 2

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background 2

representative citing papers

Stationary solutions in the small-$c$ expansion of GR

gr-qc · 2026-04-26 · conditional · novelty 7.0

The NLO/NNLO small-c (Carroll) expansion of GR admits a rich stationary vacuum sector with rotating Lense-Thirring-type, C-metric-type, Hartle-Thorne-type, and higher-multipole solutions, going beyond the static magnetic Carroll truncation.

Kerroll black holes

hep-th · 2026-05-14 · unverdicted · novelty 6.0 · 2 refs

Rotating black holes are constructed in magnetic Carroll gravity, including an intrinsically Carrollian dressed solution and a Kerroll black hole from an odd-power c-expansion of GR, with conserved charges computed.

citing papers explorer

Showing 4 of 4 citing papers.

  • Spin and Quadrupole Sectors in Nonrelativistic Gravity gr-qc · 2026-05-07 · unverdicted · none · ref 4

    Derives NLO Kerr-type and Hartle-Thorne-type solutions plus NNLO mixed spin-quadrupole solutions in the Galilean branch of nonrelativistic gravity.

  • Stationary solutions in the small-$c$ expansion of GR gr-qc · 2026-04-26 · conditional · none · ref 34

    The NLO/NNLO small-c (Carroll) expansion of GR admits a rich stationary vacuum sector with rotating Lense-Thirring-type, C-metric-type, Hartle-Thorne-type, and higher-multipole solutions, going beyond the static magnetic Carroll truncation.

  • Kerroll black holes hep-th · 2026-05-14 · unverdicted · none · ref 68 · 2 links

    Rotating black holes are constructed in magnetic Carroll gravity, including an intrinsically Carrollian dressed solution and a Kerroll black hole from an odd-power c-expansion of GR, with conserved charges computed.

  • Quantum Fluctuations and Newton-Cartan Geometry for Non-Relativistic de Sitter space hep-th · 2026-04-08 · conditional · none · ref 14

    The one-loop partition function of the Galilean-de Sitter boundary theory is Z(β) = (2/πβ²) exp(4π²c₀/β), whose β⁻² prefactor matches the four generators of the EdS-G algebra; the matching bulk is a Newton-Cartan geometry satisfying a non-relativistic JT action.