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The Super D9-Brane and its Truncations

High Energy Physics - Theory · Submitted 13 Jan 1999

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim Both of them lead to an N=1 nonlinear supersymmetrization of the D=10 cosmological constant.

how it is stated · asserted 1.00 read the record →

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arXiv IDhep-th/9901055 (version 3)
Pith IDWBRU6PK6, Pith's permanent record of this paper and its review
CitationBert Janssen, Eric Bergshoeff, Mees de Roo, Tomas Ortin. "The Super D9-Brane and its Truncations." arXiv:hep-th/9901055 (1999). https://pith.science/paper/WBRU6PK6
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What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.16 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.40 · compares with prior results 0.14 · mentions code or data availability 0.01.

The abstract, sentence by sentence

arXiv listing abstract v3. Results and the main claim are underlined; .

We consider two inequivalent truncations of the super D9--brane: the ``Heterotic'' and the ``Type I'' truncation. Both of them lead to an N=1 nonlinear supersymmetrization of the D=10 cosmological constant. The propagating degrees of freedom in the Heterotic and Type I truncation are given by the components of a D=10 vector multiplet and a single Majorana-Weyl spinor, respectively. As a by-product we find that, after the Type I truncation, the Ramond-Ramond super ten-form provides an interesting reformulation of the Volkov-Akulov action. These results can be extended to all dimensions in which spacetime filling D-branes exist, i.e. D=3,4,6 and 10.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 We consider two inequivalent truncations of the super D9--brane: the ``Heterotic'' and the ``Type I'' truncation. contribution 0.99 0.82 0.09 asserted 0.95
s1 Both of them lead to an N=1 nonlinear supersymmetrization of the D=10 cosmological constant. result 1.00 0.78 0.40 asserted 1.00
s2 The propagating degrees of freedom in the Heterotic and Type I truncation are given by the components of a D=10 vector multiplet and a single Majorana-Weyl spinor, respectively. result 1.00 0.75 0.19 asserted 1.00
s3 As a by-product we find that, after the Type I truncation, the Ramond-Ramond super ten-form provides an interesting reformulation of the Volkov-Akulov action. result 0.95 0.93 0.14 asserted 1.00
s4 These results can be extended to all dimensions in which spacetime filling D-branes exist, i.e. D=3,4,6 and 10. result 0.63 0.78 0.18 asserted 0.89

What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from proof or derivation 0.97.

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Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
Original abstract

We consider two inequivalent truncations of the super D9--brane: the ``Heterotic'' and the ``Type I'' truncation. Both of them lead to an N=1 nonlinear supersymmetrization of the D=10 cosmological constant. The propagating degrees of freedom in the Heterotic and Type I truncation are given by the components of a D=10 vector multiplet and a single Majorana-Weyl spinor, respectively. As a by-product we find that, after the Type I truncation, the Ramond-Ramond super ten-form provides an interesting reformulation of the Volkov-Akulov action. These results can be extended to all dimensions in which spacetime filling D-branes exist, i.e. D=3,4,6 and 10.

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References
How the literature uses it

8 arXiv papers cite this in 8 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

Papers citing it · 6 sentences without a confident label

Cites it as support 1 paper
  • Such a potential must exist because of T-duality, and is known to couple to the D9-branes [ref] and is required for its action to be kappa-symmetric.[As in the IIA case, more potentials than this can be defined, however they generally are not required for our purposes, though we do briefly consider a 10-form potential $B^(10)$ which should presumably appear in one of our 9-form charges.

    Topological BPS charges in 10 and 11-dimensional supergravity · Field equations in IIB Supergravity · 0.96

Cites it as background 1 paper
  • A partially “democratic” formulation of these theories, where all the RR fields are introduced together with their magnetic duals, was given in [ref] and [ref] .

    IIA/IIB Supergravity and Ten-forms · Introduction · 0.95

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