A Supersymmetric SO(10) Model with Inflation and Cosmic Strings

Rachel Jeannerot

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A Supersymmetric SO(10) Model with Inflation and Cosmic Strings

Rachel Jeannerot

High Energy Physics - Phenomenology · Submitted 22 Sep 1995

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

The authors' main claim We have built a supersymmetric SO(10) model consistent with cosmological observations.

how it is stated · asserted 0.80 read the record →

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The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

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Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 7,257 input tokens, $0.0003 reported.

What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.10 · human participants 0.01 · controlled comparison 0.01 · randomized assignment 0.01 · states quantitative result 0.08 · compares with prior results 0.07 · mentions code or data availability 0.01.

The abstract, sentence by sentence

arXiv listing abstract v2. Results and the main claim are underlined; show every role.

We have built a supersymmetric SO(10) model consistent with cosmological observations. The model gives rise to a false vacuum hybrid inflationary scenario which solves the monopole problem. We argue that this type of inflationary scenario is generic in supersymmetric SO(10) model, and arises naturally from the theory. Neither any external field nor any external symmetry has to be added. It can just be a consequence of the theory. In our specific model, at the end of inflation, cosmic strings form. The properties of the strings are presented. The cosmic background radiation anisotropies induced by the inflationary perturbations and the cosmic strings are estimated. The model produces a stable lightest superparticle and a very light left-handed neutrino which may serve as the cold and hot dark matter. The properties of a mixed cosmic string-inflationary large scale structure formation scenario are discussed.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#	sentence	role	the authors' own work	states the main conclusion	strength
s0	We have built a supersymmetric SO(10) model consistent with cosmological observations.	contribution 0.98	0.95	0.39	asserted 0.80
s1	The model gives rise to a false vacuum hybrid inflationary scenario which solves the monopole problem.	result 0.86	0.84	0.27	asserted 1.00
s2	We argue that this type of inflationary scenario is generic in supersymmetric SO(10) model, and arises naturally from the theory.	interpretation 0.98	0.52	0.31	asserted 0.75
s3	Neither any external field nor any external symmetry has to be added.	interpretation 0.58	0.41	0.09	asserted 0.98
s4	It can just be a consequence of the theory.	interpretation 0.92	0.26	0.10	hedged possibility 0.65
s5	In our specific model, at the end of inflation, cosmic strings form.	result 0.95	0.87	0.15	asserted 1.00
s6	The properties of the strings are presented.	contribution 0.82	0.82	0.05	asserted 0.77
s7	The cosmic background radiation anisotropies induced by the inflationary perturbations and the cosmic strings are estimated.	contribution 0.51	0.88	0.07	asserted 0.97
s8	The model produces a stable lightest superparticle and a very light left-handed neutrino which may serve as the cold and hot dark matter.	result 0.91	0.84	0.16	hedged possibility 0.80
s9	The properties of a mixed cosmic string-inflationary large scale structure formation scenario are discussed.	contribution 0.90	0.81	0.11	asserted 0.74

What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from proof or derivation 0.60.

What was examined, and what was not

sources read

arXiv listing abstract v2

not examined

full text
figures and tables
references and citing sentences
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S sections
T body sentences
C citations
R cross-paper relations

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 have built a supersymmetric SO(10) model consistent with cosmological observations. The model gives rise to a false vacuum hybrid inflationary scenario which solves the monopole problem. We argue that this type of inflationary scenario is generic in supersymmetric SO(10) model, and arises naturally from the theory. Neither any external field nor any external symmetry has to be added. It can just be a consequence of the theory. In our specific model, at the end of inflation, cosmic strings form. The properties of the strings are presented. The cosmic background radiation anisotropies induced by the inflationary perturbations and the cosmic strings are estimated. The model produces a stable lightest superparticle and a very light left-handed neutrino which may serve as the cold and hot dark matter. The properties of a mixed cosmic string-inflationary large scale structure formation scenario are discussed.

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References

How the literature uses it

23 arXiv papers cite this in 24 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 · 18 sentences without a confident label

Cites it as background 6 papers

For Minimal Supersymmetric $SO(10)$ GUT (MSGUT) a scenario with an embedded inflaton has been considered in a variety of contexts [ref] .

Primordial black holes from D-parity breaking in SO(10) grand unified theory · Introduction · 0.96
Cosmic strings are linear topological defects predicted by many models of particle physics that go beyond the Standard Model, e.g. in supergravity [ref] , brane inflation [ref] and "String Gas Cosmology" [ref] models.

Note on Structure Formation from Cosmic String Wakes · Introduction · 0.98
In particular, cosmic strings are predicted to form after inflation in many inflationary models, both models formulated in the context of superstring theory [ref] and in models based on supergravity [ref] .

Cosmic String Loops as the Seeds of Super-Massive Black Holes · Cosmic String Review · 0.80

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