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text stringlengths 1 1.92M | id stringlengths 14 6.21k | metadata dict |
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\section{Introduction}
\label{intro}
The astrophysical plasmas characterized by high Lundquist number
$S\equiv Lv_A/\eta$ ($L\equiv$ length scale of the magnetic field
\textbf{B} variability, $v_A\equiv$ Alfv\'en speed, and $\eta\equiv$
magnetic diffusivity) satisfy the Alfv\'en's flux-freezing theorem in presence of l... | proofpile-arXiv_065-3 | {
"file_path": "/home/ubuntu/dolma-v1_7/algebraic-stack-train-0000.json.gz"
} |
\section{Introduction}
In this paper we present and analyze a high-order time discontinuous Galerkin finite element method for the time integration of second order differential problems as those stemming from e.g. elastic wave propagation phenomena.
Classical approaches for the time integration of second order diffe... | proofpile-arXiv_065-25 | {
"file_path": "/home/ubuntu/dolma-v1_7/algebraic-stack-train-0000.json.gz"
} |
\section{Introduction}
The properties of particle interactions determine the evolution of a quantum chromodynamical (QCD) system. Thorough understanding of these properties can help answer many fundamental questions in physics, such as the origin of the Universe or the unification of forces. This is one of the importa... | proofpile-arXiv_065-32 | {
"file_path": "/home/ubuntu/dolma-v1_7/algebraic-stack-train-0000.json.gz"
} |
"\\section{Introduction}\n\\IEEEPARstart{I}{mages} captured under low-light conditions often suffer (...TRUNCATED) | proofpile-arXiv_065-35 | {
"file_path": "/home/ubuntu/dolma-v1_7/algebraic-stack-train-0000.json.gz"
} |
"\n\n\\section{Introduction}\n\\label{sect1}\n\nIn the past decades, magnetic fields in galaxy clust(...TRUNCATED) | proofpile-arXiv_065-40 | {
"file_path": "/home/ubuntu/dolma-v1_7/algebraic-stack-train-0000.json.gz"
} |
"\\section{Introduction}\n \n \n\n\t\n\n On 22 September 2017, IceCube reported a neutrino eve(...TRUNCATED) | proofpile-arXiv_065-42 | {
"file_path": "/home/ubuntu/dolma-v1_7/algebraic-stack-train-0000.json.gz"
} |
"\\section{Introduction}\\label{sec1}\nLet $\\Omega\\subseteq \\mathbb{R}^{n}~(n\\geq 2)$ be a domai(...TRUNCATED) | proofpile-arXiv_065-77 | {
"file_path": "/home/ubuntu/dolma-v1_7/algebraic-stack-train-0000.json.gz"
} |
"\\section{Introduction}\n\nHyperspectral remote sensing technology is a method that organically com(...TRUNCATED) | proofpile-arXiv_065-83 | {
"file_path": "/home/ubuntu/dolma-v1_7/algebraic-stack-train-0000.json.gz"
} |
"\\section{Introduction}\nComputed Tomography Angiography (CTA) is a commonly used modality in many (...TRUNCATED) | proofpile-arXiv_065-84 | {
"file_path": "/home/ubuntu/dolma-v1_7/algebraic-stack-train-0000.json.gz"
} |
"\\section{introduction}\n\nAssembly of galaxies in the early universe is a matter of intense debate(...TRUNCATED) | proofpile-arXiv_065-85 | {
"file_path": "/home/ubuntu/dolma-v1_7/algebraic-stack-train-0000.json.gz"
} |
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This dataset is a 10% sample of Dolma v1.7, equating to around ~305B tokens and uploaded directly as a Hugging Face dataset.
As a pure sample, it maintains the ODC-BY license.
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