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Dynamics of spinor Bose-Einstein condensate subject to dissipation

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Man-Man Pang, Yajiang Hao

Quantum Gases · Submitted 2 Feb 2016

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

The authors' main claim In contrast, the condensates subject to dissipation will not evolve along the specific dynamical orbital.

how it is stated · asserted 1.00 read the record →

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arXiv ID1602.00807 (version 1)
Pith IDQTMYDPTD, Pith's permanent record of this paper and its review
CitationMan-Man Pang, Yajiang Hao. "Dynamics of spinor Bose-Einstein condensate subject to dissipation." arXiv:1602.00807 (2016). https://pith.science/paper/QTMYDPTD
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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.

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Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,357 input tokens.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.14 · human participants 0.01 · controlled comparison 0.77 · randomized assignment 0.01 · states quantitative result 0.05 · compares with prior results 0.62 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; .

We investigate the internal dynamics of the spinor Bose-Einstein Condensates subject to dissipation by solving the Lindblad master equation. It is shown that for the condensates without dissipation its dynamics always evolve along specific orbital in the phase space of ($n_0$, $\theta$) and display three kinds of dynamical properties including Josephson-like oscillation, self-trapping-like oscillation and 'running phase'. In contrast, the condensates subject to dissipation will not evolve along the specific dynamical orbital. If component-1 and component-(-1) dissipate in different rates, the magnetization $m$ will not conserve and the system transits between different dynamical regions. The dynamical properties can be exhibited in the phase space of ($n_0$, $\theta$, $m$).

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 investigate the internal dynamics of the spinor Bose-Einstein Condensates subject to dissipation by solving the Lindblad master equation. contribution 0.70 0.94 0.07 asserted 0.94
s1 It is shown that for the condensates without dissipation its dynamics always evolve along specific orbital in the phase space of ($n_0$, $\theta$) and display three kinds of dynamical properties including Josephson-like oscillation, self-trapping-like oscillation and 'running phase'. result 0.96 0.76 0.18 asserted 1.00
s2 In contrast, the condensates subject to dissipation will not evolve along the specific dynamical orbital. result 1.00 0.83 0.33 asserted 1.00
s3 If component-1 and component-(-1) dissipate in different rates, the magnetization $m$ will not conserve and the system transits between different dynamical regions. result 1.00 0.85 0.22 asserted 0.98
s4 The dynamical properties can be exhibited in the phase space of ($n_0$, $\theta$, $m$). result 0.80 0.74 0.09 asserted 0.84

What kind of paper the classifier reports this is: theoretical result 0.66 · evidence from simulation or computation 0.72.

What was examined, and what was not

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  • figures and tables
  • references and citing sentences
  • relations to other papers
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  • P abstract
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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 investigate the internal dynamics of the spinor Bose-Einstein Condensates subject to dissipation by solving the Lindblad master equation. It is shown that for the condensates without dissipation its dynamics always evolve along specific orbital in the phase space of ($n_0$, $\theta$) and display three kinds of dynamical properties including Josephson-like oscillation, self-trapping-like oscillation and 'running phase'. In contrast, the condensates subject to dissipation will not evolve along the specific dynamical orbital. If component-1 and component-(-1) dissipate in different rates, the magnetization $m$ will not conserve and the system transits between different dynamical regions. The dynamical properties can be exhibited in the phase space of ($n_0$, $\theta$, $m$).

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