sg:pub.10.1007/s10909-014-1237-y - Springer Nature SciGraph

Article Info

DATE

2014-10-07

AUTHORS

M. Nikolo, X. Shi, E. S. Choi, J. Jiang, J. D. Weiss, E. E. Hellstrom

ABSTRACT

Flux pinning and thermally assisted flux flow are studied in a (Ba0.6\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$_{0.6}$$\end{document}K0.4)\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$_{0.4})$$\end{document}Fe2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$_{2}$$\end{document}As2(Tc\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$_{2}(T_\mathrm{c}$$\end{document}=38.3 K) bulk samples in magnetic fields up to 18 T via ac susceptibility measurements. Ac susceptibility curves shift to higher temperatures as the frequency is increased from 75 to 1,997 Hz in all fields. The frequency (f)\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$f)$$\end{document} shift of the susceptibility curves is modeled by the Anderson-Kim Arrhenius law f=f0exp(-Ea/kT)\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$f = f_{0}\mathrm{exp}(-E_\mathrm{a}{ /kT})$$\end{document} to determine flux activation energy Ea/k\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$E_\mathrm{a}/k$$\end{document} as a function of ac field Hac\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$H_\mathrm{ac}$$\end{document} and dc magnetic flux density μ\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\mu $$\end{document}0Hdc\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$_\mathrm{0} H_\mathrm{dc}$$\end{document}. Ea/k\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$E_\mathrm{a}/k$$\end{document} ranges from 8,822 K (761 meV) at μ\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\mu $$\end{document}0Hdc\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$_{0} H_{dc}$$\end{document} = 0 T to 1,100 K (95 meV) at 18 T for Hac=\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$H_\mathrm{ac}=$$\end{document}80 A/m (1 Oe). The energies drop very quickly in a non-linear manner as μ\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\mu $$\end{document}0Hdc\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$_{0} H_\mathrm{dc}$$\end{document} increases from 0 to 1 T, and more gradually, in a linear-like manner, as μ\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\mu $$\end{document}0Hdc\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$_{0} H_\mathrm{dc}$$\end{document} increases further to 18 T, suggesting some kind of vortex transition. For ac fields of 400 A/m (5 Oe) and higher, the Arrhenius model starts breaking down, at around μ\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\mu $$\end{document}0Hdc\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$_{0} H_{ \mathrm dc}$$\end{document} = 2 T. As the dc magnetic flux density increases further, this breakdown becomes significant for μ0Hdc\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\mu _{0} H_\mathrm{dc}$$\end{document} = 15 and 18 T at ac fields of 400 A/m and higher. Extensive mapping of the de-pinning, or irreversibility, lines shows broad dependence on the magnitude of the ac field, frequency, in addition to the dc magnetic flux density. More... »

PAGES

188-199

References to SciGraph publications

1996. Irreversibility Line in Superconductor as Line of Constant Shielding Current Density in ADVANCES IN CRYOGENIC ENGINEERING MATERIALS

1993. Harmonic Susceptibility and Irreversibility Line of YBa2Cu3O7 Films in ADVANCES IN SUPERCONDUCTIVITY V

Journal

TITLE

Journal of Low Temperature Physics

ISSUE

3-4

VOLUME

178

Subjects

FOR: Physical Sciences

FOR: Atomic, Molecular, Nuclear, Particle And Plasma Physics

Author Affiliations

Physics Department, Saint Louis University, 63103, St Louis, MO, USA

National High Magnetic Field Laboratory, Florida State University, 32310, Tallahassee, FL, USA

Applied Superconductivity Center, National High Magnetic Field Laboratory, Florida State University, 32310, Tallahassee, FL, USA

From Grant

National High Magnetic Field Laboratory Renewal 2013-2017

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/s10909-014-1237-y

DOI

http://dx.doi.org/10.1007/s10909-014-1237-y

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1049080081

Indexing Status Check whether this publication has been indexed by Scopus and Web Of Science using the SN Indexing Status Tool

Incoming Citations Browse incoming citations for this publication using opencitations.net

JSON-LD is the canonical representation for SciGraph data.

TIP: You can open this SciGraph record using an external JSON-LD service: JSON-LD Playground Google SDTT

[
  {
    "@context": "https://springernature.github.io/scigraph/jsonld/sgcontext.json", 
    "about": [
      {
        "id": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/02", 
        "inDefinedTermSet": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/", 
        "name": "Physical Sciences", 
        "type": "DefinedTerm"
      }, 
      {
        "id": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/0202", 
        "inDefinedTermSet": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/", 
        "name": "Atomic, Molecular, Nuclear, Particle and Plasma Physics", 
        "type": "DefinedTerm"
      }
    ], 
    "author": [
      {
        "affiliation": {
          "alternateName": "Physics Department, Saint Louis University, 63103, St Louis, MO, USA", 
          "id": "http://www.grid.ac/institutes/grid.262962.b", 
          "name": [
            "Physics Department, Saint Louis University, 63103, St Louis, MO, USA"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Nikolo", 
        "givenName": "M.", 
        "id": "sg:person.011472757650.45", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.011472757650.45"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "National High Magnetic Field Laboratory, Florida State University, 32310, Tallahassee, FL, USA", 
          "id": "http://www.grid.ac/institutes/grid.481548.4", 
          "name": [
            "National High Magnetic Field Laboratory, Florida State University, 32310, Tallahassee, FL, USA"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Shi", 
        "givenName": "X.", 
        "id": "sg:person.012261435743.14", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.012261435743.14"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "National High Magnetic Field Laboratory, Florida State University, 32310, Tallahassee, FL, USA", 
          "id": "http://www.grid.ac/institutes/grid.481548.4", 
          "name": [
            "National High Magnetic Field Laboratory, Florida State University, 32310, Tallahassee, FL, USA"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Choi", 
        "givenName": "E. S.", 
        "id": "sg:person.0635107016.86", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.0635107016.86"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "Applied Superconductivity Center, National High Magnetic Field Laboratory, Florida State University, 32310, Tallahassee, FL, USA", 
          "id": "http://www.grid.ac/institutes/grid.481548.4", 
          "name": [
            "Applied Superconductivity Center, National High Magnetic Field Laboratory, Florida State University, 32310, Tallahassee, FL, USA"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Jiang", 
        "givenName": "J.", 
        "id": "sg:person.01154110202.55", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.01154110202.55"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "Applied Superconductivity Center, National High Magnetic Field Laboratory, Florida State University, 32310, Tallahassee, FL, USA", 
          "id": "http://www.grid.ac/institutes/grid.481548.4", 
          "name": [
            "Applied Superconductivity Center, National High Magnetic Field Laboratory, Florida State University, 32310, Tallahassee, FL, USA"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Weiss", 
        "givenName": "J. D.", 
        "id": "sg:person.01056616531.73", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.01056616531.73"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "Applied Superconductivity Center, National High Magnetic Field Laboratory, Florida State University, 32310, Tallahassee, FL, USA", 
          "id": "http://www.grid.ac/institutes/grid.481548.4", 
          "name": [
            "Applied Superconductivity Center, National High Magnetic Field Laboratory, Florida State University, 32310, Tallahassee, FL, USA"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Hellstrom", 
        "givenName": "E. E.", 
        "id": "sg:person.0632002631.91", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.0632002631.91"
        ], 
        "type": "Person"
      }
    ], 
    "citation": [
      {
        "id": "sg:pub.10.1007/978-4-431-68305-6_121", 
        "sameAs": [
          "https://app.dimensions.ai/details/publication/pub.1036054329", 
          "https://doi.org/10.1007/978-4-431-68305-6_121"
        ], 
        "type": "CreativeWork"
      }, 
      {
        "id": "sg:pub.10.1007/978-1-4757-9059-7_78", 
        "sameAs": [
          "https://app.dimensions.ai/details/publication/pub.1012446158", 
          "https://doi.org/10.1007/978-1-4757-9059-7_78"
        ], 
        "type": "CreativeWork"
      }
    ], 
    "datePublished": "2014-10-07", 
    "datePublishedReg": "2014-10-07", 
    "description": "Flux pinning and thermally assisted flux flow are studied in a (Ba0.6\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$_{0.6}$$\\end{document}K0.4)\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$_{0.4})$$\\end{document}Fe2\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$_{2}$$\\end{document}As2(Tc\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$_{2}(T_\\mathrm{c}$$\\end{document}=38.3 K) bulk samples in magnetic fields up to 18 T via ac susceptibility measurements. Ac susceptibility curves shift to higher temperatures as the frequency is increased from 75 to 1,997 Hz in all fields. The frequency (f)\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$f)$$\\end{document} shift of the susceptibility curves is modeled by the Anderson-Kim Arrhenius law f=f0exp(-Ea/kT)\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$f = f_{0}\\mathrm{exp}(-E_\\mathrm{a}{ /kT})$$\\end{document} to determine flux activation energy Ea/k\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$E_\\mathrm{a}/k$$\\end{document} as a function of ac field Hac\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$H_\\mathrm{ac}$$\\end{document} and dc magnetic flux density \u03bc\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$\\mu $$\\end{document}0Hdc\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$_\\mathrm{0} H_\\mathrm{dc}$$\\end{document}. Ea/k\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$E_\\mathrm{a}/k$$\\end{document} ranges from 8,822 K (761 meV) at \u03bc\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$\\mu $$\\end{document}0Hdc\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$_{0} H_{dc}$$\\end{document} = 0 T to 1,100 K (95 meV) at 18 T for Hac=\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$H_\\mathrm{ac}=$$\\end{document}80 A/m (1 Oe). The energies drop very quickly in a non-linear manner as \u03bc\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$\\mu $$\\end{document}0Hdc\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$_{0} H_\\mathrm{dc}$$\\end{document} increases from 0 to 1 T, and more gradually, in a linear-like manner, as \u03bc\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$\\mu $$\\end{document}0Hdc\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$_{0} H_\\mathrm{dc}$$\\end{document} increases further to 18 T, suggesting some kind of vortex transition. For ac fields of 400 A/m (5 Oe) and higher, the Arrhenius model starts breaking down, at around \u03bc\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$\\mu $$\\end{document}0Hdc\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$_{0} H_{ \\mathrm dc}$$\\end{document} = 2 T. As the dc magnetic flux density increases further, this breakdown becomes significant for \u03bc0Hdc\\documentclass[12pt]{minimal}\n\t\t\t\t\\usepackage{amsmath}\n\t\t\t\t\\usepackage{wasysym}\n\t\t\t\t\\usepackage{amsfonts}\n\t\t\t\t\\usepackage{amssymb}\n\t\t\t\t\\usepackage{amsbsy}\n\t\t\t\t\\usepackage{mathrsfs}\n\t\t\t\t\\usepackage{upgreek}\n\t\t\t\t\\setlength{\\oddsidemargin}{-69pt}\n\t\t\t\t\\begin{document}$$\\mu _{0} H_\\mathrm{dc}$$\\end{document} = 15 and 18 T at ac fields of 400 A/m and higher. Extensive mapping of the de-pinning, or irreversibility, lines shows broad dependence on the magnitude of the ac field, frequency, in addition to the dc magnetic flux density.", 
    "genre": "article", 
    "id": "sg:pub.10.1007/s10909-014-1237-y", 
    "inLanguage": "en", 
    "isAccessibleForFree": false, 
    "isFundedItemOf": [
      {
        "id": "sg:grant.3479346", 
        "type": "MonetaryGrant"
      }, 
      {
        "id": "sg:grant.3113501", 
        "type": "MonetaryGrant"
      }, 
      {
        "id": "sg:grant.3484564", 
        "type": "MonetaryGrant"
      }
    ], 
    "isPartOf": [
      {
        "id": "sg:journal.1030474", 
        "issn": [
          "0022-2291", 
          "1573-7357"
        ], 
        "name": "Journal of Low Temperature Physics", 
        "publisher": "Springer Nature", 
        "type": "Periodical"
      }, 
      {
        "issueNumber": "3-4", 
        "type": "PublicationIssue"
      }, 
      {
        "type": "PublicationVolume", 
        "volumeNumber": "178"
      }
    ], 
    "keywords": [
      "magnetic flux density", 
      "ac field", 
      "flux density", 
      "linear-like manner", 
      "AC losses", 
      "flux pinning", 
      "flux flow", 
      "de-pinning", 
      "bulk superconductors", 
      "Arrhenius model", 
      "flux dynamics", 
      "activation energy", 
      "density", 
      "non-linear manner", 
      "susceptibility curves", 
      "field", 
      "energy", 
      "vortex transition", 
      "broad dependence", 
      "pinning", 
      "flow", 
      "irreversibility", 
      "superconductors", 
      "curves", 
      "Ea/", 
      "model", 
      "breakdown", 
      "extensive mapping", 
      "dependence", 
      "magnitude", 
      "frequency", 
      "increase", 
      "kind", 
      "transition", 
      "mapping", 
      "addition", 
      "dynamics", 
      "loss", 
      "shift", 
      "function", 
      "manner", 
      "lines"
    ], 
    "name": "Flux Dynamics, ac Losses, and Activation Energies in (Ba0.6K0.4)Fe2As2 Bulk Superconductor", 
    "pagination": "188-199", 
    "productId": [
      {
        "name": "dimensions_id", 
        "type": "PropertyValue", 
        "value": [
          "pub.1049080081"
        ]
      }, 
      {
        "name": "doi", 
        "type": "PropertyValue", 
        "value": [
          "10.1007/s10909-014-1237-y"
        ]
      }
    ], 
    "sameAs": [
      "https://doi.org/10.1007/s10909-014-1237-y", 
      "https://app.dimensions.ai/details/publication/pub.1049080081"
    ], 
    "sdDataset": "articles", 
    "sdDatePublished": "2022-05-20T07:29", 
    "sdLicense": "https://scigraph.springernature.com/explorer/license/", 
    "sdPublisher": {
      "name": "Springer Nature - SN SciGraph project", 
      "type": "Organization"
    }, 
    "sdSource": "s3://com-springernature-scigraph/baseset/20220519/entities/gbq_results/article/article_615.jsonl", 
    "type": "ScholarlyArticle", 
    "url": "https://doi.org/10.1007/s10909-014-1237-y"
  }
]

Download the RDF metadata as: json-ld nt turtle xml License info

HOW TO GET THIS DATA PROGRAMMATICALLY:

JSON-LD is a popular format for linked data which is fully compatible with JSON.

curl -H 'Accept: application/ld+json' 'https://scigraph.springernature.com/pub.10.1007/s10909-014-1237-y'

N-Triples is a line-based linked data format ideal for batch operations.

curl -H 'Accept: application/n-triples' 'https://scigraph.springernature.com/pub.10.1007/s10909-014-1237-y'

Turtle is a human-readable linked data format.

curl -H 'Accept: text/turtle' 'https://scigraph.springernature.com/pub.10.1007/s10909-014-1237-y'

RDF/XML is a standard XML format for linked data.

curl -H 'Accept: application/rdf+xml' 'https://scigraph.springernature.com/pub.10.1007/s10909-014-1237-y'

This table displays all metadata directly associated to this object as RDF triples.

154 TRIPLES 22 PREDICATES 69 URIs 59 LITERALS 6 BLANK NODES

	Subject	Predicate	Object
1	sg:pub.10.1007/s10909-014-1237-y	schema:about	anzsrc-for:02
2	″	″	anzsrc-for:0202
3	″	schema:author	N0717a6e630214676a093d67da4600827
4	″	schema:citation	sg:pub.10.1007/978-1-4757-9059-7_78
5	″	″	sg:pub.10.1007/978-4-431-68305-6_121
6	″	schema:datePublished	2014-10-07
7	″	schema:datePublishedReg	2014-10-07
8	″	schema:description	Flux pinning and thermally assisted flux flow are studied in a (Ba0.6\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$_{0.6}$$\end{document}K0.4)\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$_{0.4})$$\end{document}Fe2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$_{2}$$\end{document}As2(Tc\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$_{2}(T_\mathrm{c}$$\end{document}=38.3 K) bulk samples in magnetic fields up to 18 T via ac susceptibility measurements. Ac susceptibility curves shift to higher temperatures as the frequency is increased from 75 to 1,997 Hz in all fields. The frequency (f)\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$f)$$\end{document} shift of the susceptibility curves is modeled by the Anderson-Kim Arrhenius law f=f0exp(-Ea/kT)\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$f = f_{0}\mathrm{exp}(-E_\mathrm{a}{ /kT})$$\end{document} to determine flux activation energy Ea/k\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$E_\mathrm{a}/k$$\end{document} as a function of ac field Hac\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$H_\mathrm{ac}$$\end{document} and dc magnetic flux density μ\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\mu $$\end{document}0Hdc\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$_\mathrm{0} H_\mathrm{dc}$$\end{document}. Ea/k\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$E_\mathrm{a}/k$$\end{document} ranges from 8,822 K (761 meV) at μ\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\mu $$\end{document}0Hdc\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$_{0} H_{dc}$$\end{document} = 0 T to 1,100 K (95 meV) at 18 T for Hac=\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$H_\mathrm{ac}=$$\end{document}80 A/m (1 Oe). The energies drop very quickly in a non-linear manner as μ\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\mu $$\end{document}0Hdc\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$_{0} H_\mathrm{dc}$$\end{document} increases from 0 to 1 T, and more gradually, in a linear-like manner, as μ\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\mu $$\end{document}0Hdc\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$_{0} H_\mathrm{dc}$$\end{document} increases further to 18 T, suggesting some kind of vortex transition. For ac fields of 400 A/m (5 Oe) and higher, the Arrhenius model starts breaking down, at around μ\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\mu $$\end{document}0Hdc\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$_{0} H_{ \mathrm dc}$$\end{document} = 2 T. As the dc magnetic flux density increases further, this breakdown becomes significant for μ0Hdc\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\mu _{0} H_\mathrm{dc}$$\end{document} = 15 and 18 T at ac fields of 400 A/m and higher. Extensive mapping of the de-pinning, or irreversibility, lines shows broad dependence on the magnitude of the ac field, frequency, in addition to the dc magnetic flux density.
9	″	schema:genre	article
10	″	schema:inLanguage	en
11	″	schema:isAccessibleForFree	false
12	″	schema:isPartOf	N255f31d563b144e1b3cad3833280b509
13	″	″	N2b0afa7e0de94ab99c0a6af2a3caa6e4
14	″	″	sg:journal.1030474
15	″	schema:keywords	AC losses
16	″	″	Arrhenius model
17	″	″	Ea/
18	″	″	ac field
19	″	″	activation energy
20	″	″	addition
21	″	″	breakdown
22	″	″	broad dependence
23	″	″	bulk superconductors
24	″	″	curves
25	″	″	de-pinning
26	″	″	density
27	″	″	dependence
28	″	″	dynamics
29	″	″	energy
30	″	″	extensive mapping
31	″	″	field
32	″	″	flow
33	″	″	flux density
34	″	″	flux dynamics
35	″	″	flux flow
36	″	″	flux pinning
37	″	″	frequency
38	″	″	function
39	″	″	increase
40	″	″	irreversibility
41	″	″	kind
42	″	″	linear-like manner
43	″	″	lines
44	″	″	loss
45	″	″	magnetic flux density
46	″	″	magnitude
47	″	″	manner
48	″	″	mapping
49	″	″	model
50	″	″	non-linear manner
51	″	″	pinning
52	″	″	shift
53	″	″	superconductors
54	″	″	susceptibility curves
55	″	″	transition
56	″	″	vortex transition
57	″	schema:name	Flux Dynamics, ac Losses, and Activation Energies in (Ba0.6K0.4)Fe2As2 Bulk Superconductor
58	″	schema:pagination	188-199
59	″	schema:productId	N6a5f18bac5db4d85b9dc84291421e391
60	″	″	N6a7bd341686743eb919b092970df05fe
61	″	schema:sameAs	https://app.dimensions.ai/details/publication/pub.1049080081
62	″	″	https://doi.org/10.1007/s10909-014-1237-y
63	″	schema:sdDatePublished	2022-05-20T07:29
64	″	schema:sdLicense	https://scigraph.springernature.com/explorer/license/
65	″	schema:sdPublisher	Nbe254870887547329b081ebec8288eb5
66	″	schema:url	https://doi.org/10.1007/s10909-014-1237-y
67	″	sgo:license	sg:explorer/license/
68	″	sgo:sdDataset	articles
69	″	rdf:type	schema:ScholarlyArticle
70	N014d340bd376422cb21c7f206ceb2e0d	rdf:first	sg:person.0632002631.91
71	″	rdf:rest	rdf:nil
72	N0717a6e630214676a093d67da4600827	rdf:first	sg:person.011472757650.45
73	″	rdf:rest	Nefd97ee5fa2c41f19f6dddff0116a223
74	N255f31d563b144e1b3cad3833280b509	schema:volumeNumber	178
75	″	rdf:type	schema:PublicationVolume
76	N2b0afa7e0de94ab99c0a6af2a3caa6e4	schema:issueNumber	3-4
77	″	rdf:type	schema:PublicationIssue
78	N3fc7d1cfd510487ea2542460dac92d1d	rdf:first	sg:person.01154110202.55
79	″	rdf:rest	Ne7627b2113f4457b8f196c9d27d8642b
80	N6a5f18bac5db4d85b9dc84291421e391	schema:name	doi
81	″	schema:value	10.1007/s10909-014-1237-y
82	″	rdf:type	schema:PropertyValue
83	N6a7bd341686743eb919b092970df05fe	schema:name	dimensions_id
84	″	schema:value	pub.1049080081
85	″	rdf:type	schema:PropertyValue
86	Nbe254870887547329b081ebec8288eb5	schema:name	Springer Nature - SN SciGraph project
87	″	rdf:type	schema:Organization
88	Nc667cc3e6cbf4539966174fc63472e07	rdf:first	sg:person.0635107016.86
89	″	rdf:rest	N3fc7d1cfd510487ea2542460dac92d1d
90	Ne7627b2113f4457b8f196c9d27d8642b	rdf:first	sg:person.01056616531.73
91	″	rdf:rest	N014d340bd376422cb21c7f206ceb2e0d
92	Nefd97ee5fa2c41f19f6dddff0116a223	rdf:first	sg:person.012261435743.14
93	″	rdf:rest	Nc667cc3e6cbf4539966174fc63472e07
94	anzsrc-for:02	schema:inDefinedTermSet	anzsrc-for:
95	″	schema:name	Physical Sciences
96	″	rdf:type	schema:DefinedTerm
97	anzsrc-for:0202	schema:inDefinedTermSet	anzsrc-for:
98	″	schema:name	Atomic, Molecular, Nuclear, Particle and Plasma Physics
99	″	rdf:type	schema:DefinedTerm
100	sg:grant.3113501	http://pending.schema.org/fundedItem	sg:pub.10.1007/s10909-014-1237-y
101	″	rdf:type	schema:MonetaryGrant
102	sg:grant.3479346	http://pending.schema.org/fundedItem	sg:pub.10.1007/s10909-014-1237-y
103	″	rdf:type	schema:MonetaryGrant
104	sg:grant.3484564	http://pending.schema.org/fundedItem	sg:pub.10.1007/s10909-014-1237-y
105	″	rdf:type	schema:MonetaryGrant
106	sg:journal.1030474	schema:issn	0022-2291
107	″	″	1573-7357
108	″	schema:name	Journal of Low Temperature Physics
109	″	schema:publisher	Springer Nature
110	″	rdf:type	schema:Periodical
111	sg:person.01056616531.73	schema:affiliation	grid-institutes:grid.481548.4
112	″	schema:familyName	Weiss
113	″	schema:givenName	J. D.
114	″	schema:sameAs	https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.01056616531.73
115	″	rdf:type	schema:Person
116	sg:person.011472757650.45	schema:affiliation	grid-institutes:grid.262962.b
117	″	schema:familyName	Nikolo
118	″	schema:givenName	M.
119	″	schema:sameAs	https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.011472757650.45
120	″	rdf:type	schema:Person
121	sg:person.01154110202.55	schema:affiliation	grid-institutes:grid.481548.4
122	″	schema:familyName	Jiang
123	″	schema:givenName	J.
124	″	schema:sameAs	https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.01154110202.55
125	″	rdf:type	schema:Person
126	sg:person.012261435743.14	schema:affiliation	grid-institutes:grid.481548.4
127	″	schema:familyName	Shi
128	″	schema:givenName	X.
129	″	schema:sameAs	https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.012261435743.14
130	″	rdf:type	schema:Person
131	sg:person.0632002631.91	schema:affiliation	grid-institutes:grid.481548.4
132	″	schema:familyName	Hellstrom
133	″	schema:givenName	E. E.
134	″	schema:sameAs	https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.0632002631.91
135	″	rdf:type	schema:Person
136	sg:person.0635107016.86	schema:affiliation	grid-institutes:grid.481548.4
137	″	schema:familyName	Choi
138	″	schema:givenName	E. S.
139	″	schema:sameAs	https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.0635107016.86
140	″	rdf:type	schema:Person
141	sg:pub.10.1007/978-1-4757-9059-7_78	schema:sameAs	https://app.dimensions.ai/details/publication/pub.1012446158
142	″	″	https://doi.org/10.1007/978-1-4757-9059-7_78
143	″	rdf:type	schema:CreativeWork
144	sg:pub.10.1007/978-4-431-68305-6_121	schema:sameAs	https://app.dimensions.ai/details/publication/pub.1036054329
145	″	″	https://doi.org/10.1007/978-4-431-68305-6_121
146	″	rdf:type	schema:CreativeWork
147	grid-institutes:grid.262962.b	schema:alternateName	Physics Department, Saint Louis University, 63103, St Louis, MO, USA
148	″	schema:name	Physics Department, Saint Louis University, 63103, St Louis, MO, USA
149	″	rdf:type	schema:Organization
150	grid-institutes:grid.481548.4	schema:alternateName	Applied Superconductivity Center, National High Magnetic Field Laboratory, Florida State University, 32310, Tallahassee, FL, USA
151	″	″	National High Magnetic Field Laboratory, Florida State University, 32310, Tallahassee, FL, USA
152	″	schema:name	Applied Superconductivity Center, National High Magnetic Field Laboratory, Florida State University, 32310, Tallahassee, FL, USA
153	″	″	National High Magnetic Field Laboratory, Florida State University, 32310, Tallahassee, FL, USA
154	″	rdf:type	schema:Organization

Flux Dynamics, ac Losses, and Activation Energies in (Ba0.6K0.4)Fe2As2 Bulk Superconductor View Full Text