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Timelike U-dualities in Generalised Geometry
High Energy Physics - Theory · Submitted 3 Jan 2013
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim Using generalised geometry, we find that timelike U-dualities, despite previous conjectures, do not change the signature of the spacetime.
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The abstract, sentence by sentence
We study timelike U-dualities acting in three and four directions of 11-dimensional supergravity, which form the groups $SL(2)\times SL(3)$ and SL(5). Using generalised geometry, we find that timelike U-dualities, despite previous conjectures, do not change the signature of the spacetime. Furthermore, we prove that the spacetime signature must be $(-,+,...,+)$ when the U-duality modular group is either $\frac{SL(2)\times SL(3)}{SO(1,1)\times SO(2,1)}$ or $\frac{SL(5)}{SO(3,2)}$. We find that for some dual solutions it is necessary to include a trivector field which is related to the existence of non-geometric fluxes in lower dimensions. In the second part of the paper, we explicitly study the action of the dualities on supergravity solutions corresponding to M2-branes. For a finite range of the transformation, the action of $SL(2)\otimes SL(3)$ on the worldvolume of uncharged M2-branes charges them while it changes the charge of extreme M2-branes. It thus acts as a Harrison transformation. At the limits of the range, we obtain the "subtracted geometries" which correspond to an infinite Harrison boost. Outside this range the trivector field becomes non-zero and we obtain a dual solution that cannot be uniquely written in terms of a metric, 3-form and trivector. Instead it corresponds to a family of solutions linked by a local SO(1,1) rotation. The SL(5) duality is used to act on a smeared extreme M2-brane giving a brane-like solution carrying momentum in the transverse direction that the brane was delocalised along.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We study timelike U-dualities acting in three and four directions of 11-dimensional supergravity, which form the groups $SL(2)\times SL(3)$ and SL(5). | contribution 0.92 | 0.82 | 0.06 | asserted 0.99 |
| s1 | Using generalised geometry, we find that timelike U-dualities, despite previous conjectures, do not change the signature of the spacetime. | result 0.99 | 0.95 | 0.52 | asserted 1.00 |
| s2 | Furthermore, we prove that the spacetime signature must be $(-,+,...,+)$ when the U-duality modular group is either $\frac{SL(2)\times SL(3)}{SO(1,1)\times SO(2,1)}$ or $\frac{SL(5)}{SO(3,2)}$. | result 1.00 | 0.93 | 0.37 | asserted 1.00 |
| s3 | We find that for some dual solutions it is necessary to include a trivector field which is related to the existence of non-geometric fluxes in lower dimensions. | result 0.99 | 0.95 | 0.06 | asserted 0.99 |
| s4 | In the second part of the paper, we explicitly study the action of the dualities on supergravity solutions corresponding to M2-branes. | contribution 0.99 | 0.94 | 0.04 | asserted 1.00 |
| s5 | For a finite range of the transformation, the action of $SL(2)\otimes SL(3)$ on the worldvolume of uncharged M2-branes charges them while it changes the charge of extreme M2-branes. | result 1.00 | 0.93 | 0.07 | asserted 1.00 |
| s6 | It thus acts as a Harrison transformation. | interpretation 0.92 | 0.79 | 0.05 | asserted 1.00 |
| s7 | At the limits of the range, we obtain the "subtracted geometries" which correspond to an infinite Harrison boost. | result 0.97 | 0.89 | 0.05 | asserted 1.00 |
| s8 | Outside this range the trivector field becomes non-zero and we obtain a dual solution that cannot be uniquely written in terms of a metric, 3-form and trivector. | result 1.00 | 0.92 | 0.05 | asserted 1.00 |
| s9 | Instead it corresponds to a family of solutions linked by a local SO(1,1) rotation. | result 0.92 | 0.87 | 0.06 | asserted 1.00 |
| s10 | The SL(5) duality is used to act on a smeared extreme M2-brane giving a brane-like solution carrying momentum in the transverse direction that the brane was delocalised along. | result 0.82 | 0.94 | 0.08 | asserted 1.00 |
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The paper
Original abstract
We study timelike U-dualities acting in three and four directions of 11-dimensional supergravity, which form the groups $SL(2)\times SL(3)$ and SL(5). Using generalised geometry, we find that timelike U-dualities, despite previous conjectures, do not change the signature of the spacetime. Furthermore, we prove that the spacetime signature must be $(-,+,...,+)$ when the U-duality modular group is either $\frac{SL(2)\times SL(3)}{SO(1,1)\times SO(2,1)}$ or $\frac{SL(5)}{SO(3,2)}$. We find that for some dual solutions it is necessary to include a trivector field which is related to the existence of non-geometric fluxes in lower dimensions. In the second part of the paper, we explicitly study the action of the dualities on supergravity solutions corresponding to M2-branes. For a finite range of the transformation, the action of $SL(2)\otimes SL(3)$ on the worldvolume of uncharged M2-branes charges them while it changes the charge of extreme M2-branes. It thus acts as a Harrison transformation. At the limits of the range, we obtain the "subtracted geometries" which correspond to an infinite Harrison boost. Outside this range the trivector field becomes non-zero and we obtain a dual solution that cannot be uniquely written in terms of a metric, 3-form and trivector. Instead it corresponds to a family of solutions linked by a local SO(1,1) rotation. The SL(5) duality is used to act on a smeared extreme M2-brane giving a brane-like solution carrying momentum in the transverse direction that the brane was delocalised along.
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References
How the literature uses it
23 arXiv papers cite this in 33 sentences
Papers citing it · 30 sentences without a confident label
Cites it as background 3 papers
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Other interesting and relevant work on generalised geometry and double field theory can be found in [ref] .
The O_{D,D} Geometry of String Theory · Introduction · 1.00
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Let us comment more on this issue.[See [ref] for more details on the generalised metric with the Lorentzian signature.]
Non-abelian U-duality at work · Spacetime signature · 0.93
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For other related developments see also [ref] .
Subtracted Geometry from Harrison Transformations: II · Introduction and Summary · 0.99
What it cites · 49 sentences without a confident label
Contests 1 paper
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The difficulties found in the examples in [ref] are now removed, forcing us instead to describe the dual solutions using a trivector for those cases.
U-duality in three and four dimensions · Introduction · contest 0.83
Builds on 1 paper
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We can now repeat the analysis in [ref] including time amongst the dualisable coordinates in order to find the bosonic fields after the action of a duality.
U-duality in three and four dimensions · The transformation rules · 0.98
Uses the method or tool of 14 papers
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We study the action of U-dualities by using generalised geometry [ref] which makes the duality symmetries of the supergravity manifest.
U-dual fluxes and Generalized Geometry · Introduction · 1.00
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We study the action of U-dualities by using generalised geometry [ref] which makes the duality symmetries of the supergravity manifest.
Generalized Geometry and M theory · Introduction · 1.00
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We study the action of U-dualities by using generalised geometry [ref] which makes the duality symmetries of the supergravity manifest.
SO(5,5) duality in M-theory and generalized geometry · Introduction · 1.00
Compares with 1 paper
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This is the same result as obtained by Wick-rotations in [ref] and corresponds to a new extreme M2-brane of different tension and charge.
U-duality in three and four dimensions · $U_Ω$ acting on extreme M2-brane · 0.99
Cites as background 3 papers
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More details can be found in [ref] .
U-duality in three and four dimensions · Spacelike dualities · 0.98
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In particular, one may wonder what becomes of physical quantities such as mass and the 3-form charge when there is a non-zero trivector although progress has recently been made in understanding the geometry of the trivector in the context of string theory [ref] .
Non-Geometric Fluxes in Supergravity and Double Field Theory · Conclusions · 0.91
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For a comprehensive review of the Kerr/CFT correspondence, see [ref] .
The Kerr/CFT correspondence and its extensions: a comprehensive review · $U_Ω$ acting on uncharged black M2-brane · 1.00
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