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A. Bagchi, A. Mehra and P. Nandi, Field Theories with Conformal Carrollian Symmetry
Original
1901
Earlier work this paper cites.
L. Donnay and C. Marteau, Carrollian Physics at the Black Hole Horizon
Original
1903
Earlier work this paper cites.
L. Ciambelli, R. G. Leigh, C. Marteau and P. M. Petropoulos, Carroll Structures, Null Geometry and Conformal Isometries
Original
1905
Earlier work this paper cites.
A. Bagchi, A. Banerjee and P. Parekh, Tensionless Path from Closed to Open Strings
Original
1905
Earlier work this paper cites.
A. Bagchi, R. Basu, A. Mehra and P. Nandi, Field Theories on Null Manifolds
Original
1912
Earlier work this paper cites.
J. Gomis, A. Kleinschmidt, J. Palmkvist and P. Salgado-Rebolledo, Newton-Hooke/Carrollian expansions of (A)dS and Chern-Simons gravity
Original
1912
Earlier work this paper cites.
A. Ballesteros, G. Gubitosi and F. J. Herranz, Lorentzian Snyder spacetimes and their Galilei and Carroll limits from projective geometry
Original
1912
Earlier work this paper cites.
J.-M. Levy-Leblond, Une nouvelle limite non-relativiste du groupe de poincaré
1965
Earlier work this paper cites.
H. Bacry and J. Levy-Leblond, Possible kinematics
1968
Earlier work this paper cites.
M. Henneaux, Geometry of Zero Signature Space-times
1979
Earlier work this paper cites.
C. Teitelboim, The Hamiltonian Structure of Space-Time
1981
Earlier work this paper cites.
D. Hansen, J. Hartong and N. A. Obers, Non-Relativistic Gravity and its Coupling to Matter
Original
2001
Earlier work this paper cites.
A. Strominger, The dS / CFT correspondence
2001
Earlier work this paper cites.
A. Strominger, Inflation and the dS / CFT correspondence
2001
Earlier work this paper cites.
G. Gibbons, K. Hashimoto and P. Yi, Tachyon condensates, Carrollian contraction of Lorentz group, and fundamental strings
2002
Earlier work this paper cites.
E. Bergshoeff, J. M. Izquierdo and L. Romano, Carroll versus Galilei from a Brane Perspective
Original
2003
Earlier work this paper cites.
T. M. Davis and C. H. Lineweaver, Expanding confusion: common misconceptions of cosmological horizons and the superluminal expansion of the universe
2004
Earlier work this paper cites.
L. Ciambelli, C. Marteau, P. M. Petropoulos and R. Ruzziconi, Gauges in Three-Dimensional Gravity and Holographic Fluids
Original
2006
Earlier work this paper cites.

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Then

G. Festuccia, D. Hansen, J. Hartong and N. A. Obers, Torsional Newton-Cartan Geometry from the Noether Procedure
Original
2016
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2017
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E. Bergshoeff, J. Gomis, B. Rollier, J. Rosseel and T. ter Veldhuis, Carroll versus Galilei Gravity
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C. Duval, G. W. Gibbons, P. A. Horvathy and P. M. Zhang, Carroll symmetry of plane gravitational waves

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2021

Carroll symmetry, dark energy and inflation

de Boer, Jan, Hartong, Jelle, Obers, Niels A. et al.

Understand

Carroll symmetry arises from Poincar\'e symmetry upon taking the limit of vanishing speed of light.

We determine the constraints on the energy-momentum tensor implied by Carroll symmetry and show that for energy-momentum tensors of perfect fluid form, these imply an equation of state ${\cal E}+P=0$ for energy density plus pressure.
Therefore Carroll symmetry might be relevant for dark energy and inflation.
In the Carroll limit, the Hubble radius goes to zero and outside it recessional velocities are naturally large compared to the speed of light.