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Stellar Dynamics and Black Holes

Astrophysics of Galaxies · Submitted 28 Mar 2011

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

The authors' main claim Chandrasekhar's most important contribution to stellar dynamics was the concept of dynamical friction.

how it is stated · asserted 1.00 read the record →

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arXiv ID1103.5446 (version 2)
Pith ID7K2H34WB, Pith's permanent record of this paper and its review
CitationDavid Merritt. "Stellar Dynamics and Black Holes." arXiv:1103.5446 (2011). https://pith.science/paper/7K2H34WB
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, 2,224 input tokens, $0.0001 reported.

What the abstract itself states, as probabilities: claims first 0.07 · states limitation 0.09 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.03 · compares with prior results 0.09 · mentions code or data availability 0.02.

The abstract, sentence by sentence

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

Chandrasekhar's most important contribution to stellar dynamics was the concept of dynamical friction. I briefly review that work, then discuss some implications of Chandrasekhar's theory of gravitational encounters for motion in galactic nuclei.

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 Chandrasekhar's most important contribution to stellar dynamics was the concept of dynamical friction. background 0.98 0.03 0.23 asserted 1.00
s1 I briefly review that work, then discuss some implications of Chandrasekhar's theory of gravitational encounters for motion in galactic nuclei. contribution 0.82 0.47 0.08 unclear 0.51

What kind of paper the classifier reports this is: review 0.98 · evidence from literature 0.83.

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

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

Chandrasekhar's most important contribution to stellar dynamics was the concept of dynamical friction. I briefly review that work, then discuss some implications of Chandrasekhar's theory of gravitational encounters for motion in galactic nuclei.

Human review

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