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proofpile-arXiv_065-135 |
\section{Introduction}
\label{sec:intro}
Interactions of cosmic-ray particles with detector materials can produce radioactive isotopes that create backgrounds for experiments searching for rare events such as dark matter interactions and neutrinoless double beta decay. Silicon is a widely used detector material becaus... | 2024-02-18T23:39:40.337Z | 2020-11-24T02:21:07.000Z | algebraic_stack_train_0000 | 22 | 14,429 | |
proofpile-arXiv_065-241 | \section{Motivation}
Chromium is considered as the archetypical itinerant antiferromagnet~\cite{1988_Fawcett_RevModPhys, 1994_Fawcett_RevModPhys}. Interestingly, it shares its body-centered cubic crystal structure $Im\overline{3}m$ with the archetypical itinerant ferromagnet $\alpha$-iron and, at melting temperature, ... | 2024-02-18T23:39:40.791Z | 2020-07-22T02:11:10.000Z | algebraic_stack_train_0000 | 45 | 9,343 | |
proofpile-arXiv_065-258 | "\\section{Introduction}\nWith technological advancements in the automotive industry in recent times(...TRUNCATED) | 2024-02-18T23:39:40.868Z | 2020-07-22T02:06:02.000Z | algebraic_stack_train_0000 | 50 | 7,840 | |
proofpile-arXiv_065-297 | "\\section{Introduction}\n\\label{sec:start}\n\n\\subsection{The landscape}\\label{sect:landsc}\n\nI(...TRUNCATED) | 2024-02-18T23:39:40.993Z | 2021-05-07T02:21:39.000Z | algebraic_stack_train_0000 | 58 | 31,462 | |
proofpile-arXiv_065-337 | "\\section{Introduction}\nFirst-principles calculations based on density functional \ntheory~\\cite{(...TRUNCATED) | 2024-02-18T23:39:41.175Z | 1996-09-20T17:30:30.000Z | algebraic_stack_train_0000 | 66 | 6,802 | |
proofpile-arXiv_065-359 | "\\section{Why should we study rare charm decays? }\nAt HERA recent measurements of the charm produc(...TRUNCATED) | 2024-02-18T23:39:41.244Z | 1996-09-12T17:37:21.000Z | algebraic_stack_train_0000 | 71 | 5,262 | |
proofpile-arXiv_065-513 | "\\section{Introduction}\n\\renewcommand{\\theequation}{\\thesection.\\arabic{equation}}\n\nIt is we(...TRUNCATED) | 2024-02-18T23:39:41.757Z | 1996-09-06T02:43:49.000Z | algebraic_stack_train_0000 | 96 | 10,474 | |
proofpile-arXiv_065-524 | "\\section*{Acknowledgments}\n\nWe are grateful to V.A. Kuzmin and M.A. Shifman for useful\ndiscussi(...TRUNCATED) | 2024-02-18T23:39:41.792Z | 1996-09-22T14:34:57.000Z | algebraic_stack_train_0000 | 100 | 109 | |
proofpile-arXiv_065-547 | "\\section{Introduction}\n\nLate-type Low Surface Brightness galaxies (LSBs) are considered to be ve(...TRUNCATED) | 2024-02-18T23:39:41.852Z | 1996-09-12T21:33:37.000Z | algebraic_stack_train_0000 | 105 | 2,412 | |
proofpile-arXiv_065-600 | "\\section{Introduction}\n\nIrrotational dust spacetimes have been widely studied, in\nparticular as(...TRUNCATED) | 2024-02-18T23:39:41.996Z | 1996-09-30T12:38:02.000Z | algebraic_stack_train_0000 | 115 | 3,577 |
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