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High Energy Physics - Phenomenology · arXiv:hep-ph/0308211 v2 · submitted 20 Aug 2003

Absence of isentropic expansion in various inflation models

Arjun Berera, Rudnei O. Ramos

The paper says

“Thus, for many inflation models, believed to yield exclusively isentropic inflation, the parameter space now divides into regimes of isentropic and nonisentropic inflation.”

from the abstract · picked out as the main claim by a classifier

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The paper

Abstract

Dynamics of the inflaton is studied when it interacts with boson and fermion fields and in minimal supersymmetric models. This encompasses multifield inflation models, such as hybrid inflation, and typical reheating models. For much of the parameter space conducive to inflation, the inflaton is found to dissipate adequate radiation to have observational effects on density perturbations and in cases to significantly affect inflaton evolution. Thus, for many inflation models, believed to yield exclusively isentropic inflation, the parameter space now divides into regimes of isentropic and nonisentropic inflation.

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

How the main claim is stated: asserted 0.96

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.16 · human participants 0.01 · controlled comparison 0.05 · randomized assignment 0.01 · states quantitative result 0.05 · compares with prior results 0.37 · mentions code or data availability 0.01

The abstract, sentence by sentence

This table labels the abstract only (arXiv listing abstract v2). The number is the probability the classifier gave the label.

SentenceRoleThe authors' own workStates the main conclusionStrength
Dynamics of the inflaton is studied when it interacts with boson and fermion fields and in minimal supersymmetric models. contribution 0.95 0.70 0.03 asserted 0.85
This encompasses multifield inflation models, such as hybrid inflation, and typical reheating models. background 0.60 0.15 0.03 asserted 0.99
For much of the parameter space conducive to inflation, the inflaton is found to dissipate adequate radiation to have observational effects on density perturbations and in cases to significantly affect inflaton evolution. result 1.00 0.88 0.29 asserted 0.99
Thus, for many inflation models, believed to yield exclusively isentropic inflation, the parameter space now divides into regimes of isentropic and nonisentropic inflation. interpretation 0.93 0.59 0.83 asserted 0.96

What kind of paper the classifier reports this is: theoretical result 0.97 · evidence from proof or derivation 0.77

What was examined, and what was not

Sources read

  • arXiv listing abstract v2

Not examined

  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers

Levels run

  • P abstract

Not run

  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

How the labels were made

Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 3,600 input tokens, $0.0002 reported.

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. This record as JSON

Cited by 6 Pith papers
How the literature uses it

7 arXiv papers cite this in 12 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 · 8 sentences without a confident label

Cites it as background 4 papers
  • Most scenarios considered in the literature so far in the context of quantum field theory [ref] , as well as phenomenological models [ref] consider the case where a nearly-thermal bath of radiation is produced concurrently with accelerated expansion from the adiabatic motion of the inflaton field, which may be analyzed within the framework of linear response theory.

    Warm Inflection · Introduction · 0.93

  • Although there are other models protecting quantum and thermal corrections to the inflaton potential [ref] , we focus on the minimal warm inflation model in this paper.

    Chromo-natural warm inflation · A review of minimal warm inflation · 0.90

  • This scenario constitutes the first successful implementation of warm inflation within a concrete extension of the SM, building upon a large body of work over the past decades in terms of understanding the intricacies of non-equilibrium processes during inflation [ref] , model building [ref] and observational predictions [ref] .

    Warm Inflation, Neutrinos and Dark matter: a minimal extension of the Standard Model · Introduction · 0.90

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