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Inflaton Particles in Reheating

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A. B. Henriques, R. G. Moorhouse

High Energy Physics - Phenomenology · Submitted 5 Jul 2000

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

The authors' main claim In particular we consider effects on the long-wavelength curvature parameter relevant to the cosmic microwave background fluctuations.

how it is stated · unclear 0.54 read the record →

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arXiv IDhep-ph/0007043 (version 4)
Pith IDJUXIXG3V, Pith's permanent record of this paper and its review
CitationA. B. Henriques, R. G. Moorhouse. "Inflaton Particles in Reheating." arXiv:hep-ph/0007043 (2000). https://pith.science/paper/JUXIXG3V
Claim paper

The compiled record

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.

Open the compiled record

Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 2,918 input tokens, $0.0001 reported.

What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.21 · human participants 0.01 · controlled comparison 0.18 · randomized assignment 0.01 · states quantitative result 0.03 · compares with prior results 0.45 · mentions code or data availability 0.01.

The abstract, sentence by sentence

arXiv listing abstract v4. Results and the main claim are underlined; .

In many theories of reheating starting from the classical spatially homogeneous inflaton field, its accompanying inhomogeneous part (which arises from primordial quantum fluctuations) is treated as a first order perturbation. We examine some consequences of treating it non-perturbatively in a model where a first order treatment is invalid. In particular we consider effects on the long-wavelength curvature parameter relevant to the cosmic microwave background fluctuations.

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 In many theories of reheating starting from the classical spatially homogeneous inflaton field, its accompanying inhomogeneous part (which arises from primordial quantum fluctuations) is treated as a first order perturbation. background 1.00 0.05 0.03 asserted 0.98
s1 We examine some consequences of treating it non-perturbatively in a model where a first order treatment is invalid. contribution 0.99 0.87 0.11 asserted 0.79
s2 In particular we consider effects on the long-wavelength curvature parameter relevant to the cosmic microwave background fluctuations. contribution 0.97 0.68 0.12 unclear 0.54

What kind of paper the classifier reports this is: theoretical result 0.97 · evidence from proof or derivation 0.63.

What was examined, and what was not

sources read
  • arXiv listing abstract v4
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

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

In many theories of reheating starting from the classical spatially homogeneous inflaton field, its accompanying inhomogeneous part (which arises from primordial quantum fluctuations) is treated as a first order perturbation. We examine some consequences of treating it non-perturbatively in a model where a first order treatment is invalid. In particular we consider effects on the long-wavelength curvature parameter relevant to the cosmic microwave background fluctuations.

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