Cosmic-ray-induced 63Ni --A potential confounder of fast-neutron-induced 63Ni in copper samples from Hiroshima View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2003-08

AUTHORS

W. Rühm, G. Rugel, T. Faestermann, K. Knie, A. Wallner, B. Heisinger, E. Nolte, A.A. Marchetti, R.E. Martinelli, K.L. Carroll, G. Korschinek

ABSTRACT

.Recently, the determination of 63Ni in copper samples has been suggested as a means to assess fast-neutron fluences in Hiroshima and Nagasaki. In those samples, 63Ni (half-life: 100.07 years) was produced by MeV neutrons from the A-bomb explosions via the reaction 63Cu(n,p)63Ni. For large distances from the hypocenters, cosmic-ray-induced production of 63Ni might also be important and, therefore, it is calculated here. The effective probability f* which is required to quantify the cosmic-ray-induced production by stopped muons, was measured, and a value of (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$12.6 \pm 1.6$\end{document})% obtained. The cross-section for the cosmic-ray-induced production by fast muons was measured to be (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$0.64 \pm 0.33$\end{document}) mb, at a muon energy of 100 GeV. To validate the proposed method, cosmic-ray-induced production of 32P in sulfur and of 39Ar in granite was also calculated, and reasonable agreement with literature values was found. Our estimates indicate that as many as \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$(4 -5)\cdot 10^{3}$\end{document}63Ni nuclei per gram copper were produced in a sample that was exposed to cosmic radiation in Hiroshima for about 80 years. A similar concentration due to A-bomb neutrons would be expected in Hiroshima at a distance from the hypocenter of about 1900 m. More... »

PAGES

633-639

References to SciGraph publications

Identifiers

URI

http://scigraph.springernature.com/pub.10.1140/epja/i2003-10034-2

DOI

http://dx.doi.org/10.1140/epja/i2003-10034-2

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1007069119


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/2008/0299", 
        "inDefinedTermSet": "http://purl.org/au-research/vocabulary/anzsrc-for/2008/", 
        "name": "Other Physical Sciences", 
        "type": "DefinedTerm"
      }
    ], 
    "author": [
      {
        "affiliation": {
          "alternateName": "Radiobiological Institute, University of Munich, Schillerstrasse 42, 80336, Munich, Germany", 
          "id": "http://www.grid.ac/institutes/grid.5252.0", 
          "name": [
            "Radiobiological Institute, University of Munich, Schillerstrasse 42, 80336, Munich, Germany"
          ], 
          "type": "Organization"
        }, 
        "familyName": "R\u00fchm", 
        "givenName": "W.", 
        "id": "sg:person.0712243032.64", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.0712243032.64"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "Maier-Leibnitz Laboratory, Faculty of Physics, Technical University of Munich, 85747, Garching, Germany", 
          "id": "http://www.grid.ac/institutes/grid.6936.a", 
          "name": [
            "Radiobiological Institute, University of Munich, Schillerstrasse 42, 80336, Munich, Germany", 
            "Maier-Leibnitz Laboratory, Faculty of Physics, Technical University of Munich, 85747, Garching, Germany"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Rugel", 
        "givenName": "G.", 
        "id": "sg:person.0770662011.44", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.0770662011.44"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "Maier-Leibnitz Laboratory, Faculty of Physics, Technical University of Munich, 85747, Garching, Germany", 
          "id": "http://www.grid.ac/institutes/grid.6936.a", 
          "name": [
            "Maier-Leibnitz Laboratory, Faculty of Physics, Technical University of Munich, 85747, Garching, Germany"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Faestermann", 
        "givenName": "T.", 
        "id": "sg:person.0643451432.77", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.0643451432.77"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "Maier-Leibnitz Laboratory, Faculty of Physics, Technical University of Munich, 85747, Garching, Germany", 
          "id": "http://www.grid.ac/institutes/grid.6936.a", 
          "name": [
            "Maier-Leibnitz Laboratory, Faculty of Physics, Technical University of Munich, 85747, Garching, Germany"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Knie", 
        "givenName": "K.", 
        "id": "sg:person.010533332553.16", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.010533332553.16"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "Maier-Leibnitz Laboratory, Faculty of Physics, Technical University of Munich, 85747, Garching, Germany", 
          "id": "http://www.grid.ac/institutes/grid.6936.a", 
          "name": [
            "Radiobiological Institute, University of Munich, Schillerstrasse 42, 80336, Munich, Germany", 
            "Maier-Leibnitz Laboratory, Faculty of Physics, Technical University of Munich, 85747, Garching, Germany"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Wallner", 
        "givenName": "A.", 
        "id": "sg:person.0640760464.11", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.0640760464.11"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "Maier-Leibnitz Laboratory, Faculty of Physics, Technical University of Munich, 85747, Garching, Germany", 
          "id": "http://www.grid.ac/institutes/grid.6936.a", 
          "name": [
            "Maier-Leibnitz Laboratory, Faculty of Physics, Technical University of Munich, 85747, Garching, Germany"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Heisinger", 
        "givenName": "B.", 
        "id": "sg:person.011024414135.09", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.011024414135.09"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "Maier-Leibnitz Laboratory, Faculty of Physics, Technical University of Munich, 85747, Garching, Germany", 
          "id": "http://www.grid.ac/institutes/grid.6936.a", 
          "name": [
            "Maier-Leibnitz Laboratory, Faculty of Physics, Technical University of Munich, 85747, Garching, Germany"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Nolte", 
        "givenName": "E.", 
        "id": "sg:person.0737273127.46", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.0737273127.46"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "Maier-Leibnitz Laboratory, Faculty of Physics", 
          "id": "http://www.grid.ac/institutes/None", 
          "name": [
            "Maier-Leibnitz Laboratory, Faculty of Physics"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Marchetti", 
        "givenName": "A.A.", 
        "id": "sg:person.0654433411.29", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.0654433411.29"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "Maier-Leibnitz Laboratory, Faculty of Physics", 
          "id": "http://www.grid.ac/institutes/None", 
          "name": [
            "Maier-Leibnitz Laboratory, Faculty of Physics"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Martinelli", 
        "givenName": "R.E.", 
        "id": "sg:person.016051353473.11", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.016051353473.11"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "Maier-Leibnitz Laboratory, Faculty of Physics", 
          "id": "http://www.grid.ac/institutes/None", 
          "name": [
            "Maier-Leibnitz Laboratory, Faculty of Physics"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Carroll", 
        "givenName": "K.L.", 
        "id": "sg:person.01002700706.77", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.01002700706.77"
        ], 
        "type": "Person"
      }, 
      {
        "affiliation": {
          "alternateName": "Maier-Leibnitz Laboratory, Faculty of Physics, Technical University of Munich, 85747, Garching, Germany", 
          "id": "http://www.grid.ac/institutes/grid.6936.a", 
          "name": [
            "Maier-Leibnitz Laboratory, Faculty of Physics, Technical University of Munich, 85747, Garching, Germany"
          ], 
          "type": "Organization"
        }, 
        "familyName": "Korschinek", 
        "givenName": "G.", 
        "id": "sg:person.0703577227.54", 
        "sameAs": [
          "https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.0703577227.54"
        ], 
        "type": "Person"
      }
    ], 
    "citation": [
      {
        "id": "sg:pub.10.1007/s004110050131", 
        "sameAs": [
          "https://app.dimensions.ai/details/publication/pub.1037305224", 
          "https://doi.org/10.1007/s004110050131"
        ], 
        "type": "CreativeWork"
      }
    ], 
    "datePublished": "2003-08", 
    "datePublishedReg": "2003-08-01", 
    "description": "Abstract.Recently, the determination of 63Ni in copper samples has been suggested as a means to assess fast-neutron fluences in Hiroshima and Nagasaki. In those samples, 63Ni (half-life: 100.07 years) was produced by MeV neutrons from the A-bomb explosions via the reaction 63Cu(n,p)63Ni. For large distances from the hypocenters, cosmic-ray-induced production of 63Ni might also be important and, therefore, it is calculated here. The effective probability f* which is required to quantify the cosmic-ray-induced production by stopped muons, was measured, and a value of (\\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}$12.6 \\pm 1.6$\\end{document})% obtained. The cross-section for the cosmic-ray-induced production by fast muons was measured to be (\\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}$0.64 \\pm 0.33$\\end{document}) mb, at a muon energy of 100 GeV. To validate the proposed method, cosmic-ray-induced production of 32P in sulfur and of 39Ar in granite was also calculated, and reasonable agreement with literature values was found. Our estimates indicate that as many as \\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}$(4 -5)\\cdot 10^{3}$\\end{document}63Ni nuclei per gram copper were produced in a sample that was exposed to cosmic radiation in Hiroshima for about 80 years. A similar concentration due to A-bomb neutrons would be expected in Hiroshima at a distance from the hypocenter of about 1900 m.", 
    "genre": "article", 
    "id": "sg:pub.10.1140/epja/i2003-10034-2", 
    "inLanguage": "en", 
    "isAccessibleForFree": false, 
    "isPartOf": [
      {
        "id": "sg:journal.1313769", 
        "issn": [
          "1434-6001", 
          "1434-601X"
        ], 
        "name": "The European Physical Journal A", 
        "publisher": "Springer Nature", 
        "type": "Periodical"
      }, 
      {
        "issueNumber": "4", 
        "type": "PublicationIssue"
      }, 
      {
        "type": "PublicationVolume", 
        "volumeNumber": "17"
      }
    ], 
    "keywords": [
      "cosmic radiation", 
      "copper samples", 
      "muon energy", 
      "fast-neutron fluence", 
      "MeV neutrons", 
      "fast muons", 
      "large distances", 
      "muons", 
      "bomb neutrons", 
      "neutrons", 
      "reasonable agreement", 
      "fluence", 
      "literature values", 
      "radiation", 
      "energy", 
      "distance", 
      "nucleus", 
      "explosion", 
      "agreement", 
      "samples", 
      "Hiroshima", 
      "determination", 
      "reaction", 
      "values", 
      "MB", 
      "copper", 
      "sulfur", 
      "means", 
      "production", 
      "method", 
      "Nagasaki", 
      "estimates", 
      "probability f", 
      "concentration", 
      "bomb explosion", 
      "hypocenters", 
      "similar concentrations", 
      "years", 
      "granite", 
      "determination of 63Ni", 
      "potential confounders", 
      "confounders", 
      "production of 63Ni", 
      "effective probability f"
    ], 
    "name": "Cosmic-ray-induced 63Ni --A potential confounder of fast-neutron-induced 63Ni in copper samples from Hiroshima", 
    "pagination": "633-639", 
    "productId": [
      {
        "name": "dimensions_id", 
        "type": "PropertyValue", 
        "value": [
          "pub.1007069119"
        ]
      }, 
      {
        "name": "doi", 
        "type": "PropertyValue", 
        "value": [
          "10.1140/epja/i2003-10034-2"
        ]
      }
    ], 
    "sameAs": [
      "https://doi.org/10.1140/epja/i2003-10034-2", 
      "https://app.dimensions.ai/details/publication/pub.1007069119"
    ], 
    "sdDataset": "articles", 
    "sdDatePublished": "2021-12-01T19:14", 
    "sdLicense": "https://scigraph.springernature.com/explorer/license/", 
    "sdPublisher": {
      "name": "Springer Nature - SN SciGraph project", 
      "type": "Organization"
    }, 
    "sdSource": "s3://com-springernature-scigraph/baseset/20211201/entities/gbq_results/article/article_372.jsonl", 
    "type": "ScholarlyArticle", 
    "url": "https://doi.org/10.1140/epja/i2003-10034-2"
  }
]
 

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.10.1140/epja/i2003-10034-2'

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

curl -H 'Accept: application/n-triples' 'https://scigraph.springernature.com/pub.10.1140/epja/i2003-10034-2'

Turtle is a human-readable linked data format.

curl -H 'Accept: text/turtle' 'https://scigraph.springernature.com/pub.10.1140/epja/i2003-10034-2'

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

curl -H 'Accept: application/rdf+xml' 'https://scigraph.springernature.com/pub.10.1140/epja/i2003-10034-2'


 

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

183 TRIPLES      22 PREDICATES      71 URIs      62 LITERALS      6 BLANK NODES

Subject Predicate Object
1 sg:pub.10.1140/epja/i2003-10034-2 schema:about anzsrc-for:02
2 anzsrc-for:0299
3 schema:author N581104e1ab444ee894486f2ca78d2b97
4 schema:citation sg:pub.10.1007/s004110050131
5 schema:datePublished 2003-08
6 schema:datePublishedReg 2003-08-01
7 schema:description Abstract.Recently, the determination of 63Ni in copper samples has been suggested as a means to assess fast-neutron fluences in Hiroshima and Nagasaki. In those samples, 63Ni (half-life: 100.07 years) was produced by MeV neutrons from the A-bomb explosions via the reaction 63Cu(n,p)63Ni. For large distances from the hypocenters, cosmic-ray-induced production of 63Ni might also be important and, therefore, it is calculated here. The effective probability f* which is required to quantify the cosmic-ray-induced production by stopped muons, was measured, and a value of (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$12.6 \pm 1.6$\end{document})% obtained. The cross-section for the cosmic-ray-induced production by fast muons was measured to be (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$0.64 \pm 0.33$\end{document}) mb, at a muon energy of 100 GeV. To validate the proposed method, cosmic-ray-induced production of 32P in sulfur and of 39Ar in granite was also calculated, and reasonable agreement with literature values was found. Our estimates indicate that as many as \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$(4 -5)\cdot 10^{3}$\end{document}63Ni nuclei per gram copper were produced in a sample that was exposed to cosmic radiation in Hiroshima for about 80 years. A similar concentration due to A-bomb neutrons would be expected in Hiroshima at a distance from the hypocenter of about 1900 m.
8 schema:genre article
9 schema:inLanguage en
10 schema:isAccessibleForFree false
11 schema:isPartOf N4497ab73596e44d78d45727f84ed8d8e
12 Na4de2e288df2447db2b46a0bcb973b2e
13 sg:journal.1313769
14 schema:keywords Hiroshima
15 MB
16 MeV neutrons
17 Nagasaki
18 agreement
19 bomb explosion
20 bomb neutrons
21 concentration
22 confounders
23 copper
24 copper samples
25 cosmic radiation
26 determination
27 determination of 63Ni
28 distance
29 effective probability f
30 energy
31 estimates
32 explosion
33 fast muons
34 fast-neutron fluence
35 fluence
36 granite
37 hypocenters
38 large distances
39 literature values
40 means
41 method
42 muon energy
43 muons
44 neutrons
45 nucleus
46 potential confounders
47 probability f
48 production
49 production of 63Ni
50 radiation
51 reaction
52 reasonable agreement
53 samples
54 similar concentrations
55 sulfur
56 values
57 years
58 schema:name Cosmic-ray-induced 63Ni --A potential confounder of fast-neutron-induced 63Ni in copper samples from Hiroshima
59 schema:pagination 633-639
60 schema:productId N17dc850c1e334e1abbba61519e5f6e08
61 Nf49bb8cc567441fbba40c8b4bd2d5909
62 schema:sameAs https://app.dimensions.ai/details/publication/pub.1007069119
63 https://doi.org/10.1140/epja/i2003-10034-2
64 schema:sdDatePublished 2021-12-01T19:14
65 schema:sdLicense https://scigraph.springernature.com/explorer/license/
66 schema:sdPublisher N755b124a4aba4d149ca415490e2ea138
67 schema:url https://doi.org/10.1140/epja/i2003-10034-2
68 sgo:license sg:explorer/license/
69 sgo:sdDataset articles
70 rdf:type schema:ScholarlyArticle
71 N0acaee632cf7463d80ac410661738cf8 rdf:first sg:person.0640760464.11
72 rdf:rest N2f26ec8b56624b9e82fea06b56156fda
73 N0b5b35c7f83e4c068ee6fcd85aae8dda rdf:first sg:person.0643451432.77
74 rdf:rest Nb66f7905c5b844389a7afa33bb0b337e
75 N17dc850c1e334e1abbba61519e5f6e08 schema:name doi
76 schema:value 10.1140/epja/i2003-10034-2
77 rdf:type schema:PropertyValue
78 N2f26ec8b56624b9e82fea06b56156fda rdf:first sg:person.011024414135.09
79 rdf:rest N3fb72e526ee449daa23b2b365337d8fa
80 N3fb72e526ee449daa23b2b365337d8fa rdf:first sg:person.0737273127.46
81 rdf:rest Nbeb1c8172d4645cea6643a965c66e849
82 N4497ab73596e44d78d45727f84ed8d8e schema:volumeNumber 17
83 rdf:type schema:PublicationVolume
84 N581104e1ab444ee894486f2ca78d2b97 rdf:first sg:person.0712243032.64
85 rdf:rest Na232017a3395400eb2d86bd1f539deb9
86 N6d49f8eae8c4491cb06d5c9993ff6229 rdf:first sg:person.016051353473.11
87 rdf:rest Nfd05e3f2e507440f8b148a25d5db3d4e
88 N6fcfa718d5cd47eab3963d9b6ee8c60d rdf:first sg:person.0703577227.54
89 rdf:rest rdf:nil
90 N755b124a4aba4d149ca415490e2ea138 schema:name Springer Nature - SN SciGraph project
91 rdf:type schema:Organization
92 Na232017a3395400eb2d86bd1f539deb9 rdf:first sg:person.0770662011.44
93 rdf:rest N0b5b35c7f83e4c068ee6fcd85aae8dda
94 Na4de2e288df2447db2b46a0bcb973b2e schema:issueNumber 4
95 rdf:type schema:PublicationIssue
96 Nb66f7905c5b844389a7afa33bb0b337e rdf:first sg:person.010533332553.16
97 rdf:rest N0acaee632cf7463d80ac410661738cf8
98 Nbeb1c8172d4645cea6643a965c66e849 rdf:first sg:person.0654433411.29
99 rdf:rest N6d49f8eae8c4491cb06d5c9993ff6229
100 Nf49bb8cc567441fbba40c8b4bd2d5909 schema:name dimensions_id
101 schema:value pub.1007069119
102 rdf:type schema:PropertyValue
103 Nfd05e3f2e507440f8b148a25d5db3d4e rdf:first sg:person.01002700706.77
104 rdf:rest N6fcfa718d5cd47eab3963d9b6ee8c60d
105 anzsrc-for:02 schema:inDefinedTermSet anzsrc-for:
106 schema:name Physical Sciences
107 rdf:type schema:DefinedTerm
108 anzsrc-for:0299 schema:inDefinedTermSet anzsrc-for:
109 schema:name Other Physical Sciences
110 rdf:type schema:DefinedTerm
111 sg:journal.1313769 schema:issn 1434-6001
112 1434-601X
113 schema:name The European Physical Journal A
114 schema:publisher Springer Nature
115 rdf:type schema:Periodical
116 sg:person.01002700706.77 schema:affiliation grid-institutes:None
117 schema:familyName Carroll
118 schema:givenName K.L.
119 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.01002700706.77
120 rdf:type schema:Person
121 sg:person.010533332553.16 schema:affiliation grid-institutes:grid.6936.a
122 schema:familyName Knie
123 schema:givenName K.
124 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.010533332553.16
125 rdf:type schema:Person
126 sg:person.011024414135.09 schema:affiliation grid-institutes:grid.6936.a
127 schema:familyName Heisinger
128 schema:givenName B.
129 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.011024414135.09
130 rdf:type schema:Person
131 sg:person.016051353473.11 schema:affiliation grid-institutes:None
132 schema:familyName Martinelli
133 schema:givenName R.E.
134 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.016051353473.11
135 rdf:type schema:Person
136 sg:person.0640760464.11 schema:affiliation grid-institutes:grid.6936.a
137 schema:familyName Wallner
138 schema:givenName A.
139 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.0640760464.11
140 rdf:type schema:Person
141 sg:person.0643451432.77 schema:affiliation grid-institutes:grid.6936.a
142 schema:familyName Faestermann
143 schema:givenName T.
144 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.0643451432.77
145 rdf:type schema:Person
146 sg:person.0654433411.29 schema:affiliation grid-institutes:None
147 schema:familyName Marchetti
148 schema:givenName A.A.
149 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.0654433411.29
150 rdf:type schema:Person
151 sg:person.0703577227.54 schema:affiliation grid-institutes:grid.6936.a
152 schema:familyName Korschinek
153 schema:givenName G.
154 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.0703577227.54
155 rdf:type schema:Person
156 sg:person.0712243032.64 schema:affiliation grid-institutes:grid.5252.0
157 schema:familyName Rühm
158 schema:givenName W.
159 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.0712243032.64
160 rdf:type schema:Person
161 sg:person.0737273127.46 schema:affiliation grid-institutes:grid.6936.a
162 schema:familyName Nolte
163 schema:givenName E.
164 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.0737273127.46
165 rdf:type schema:Person
166 sg:person.0770662011.44 schema:affiliation grid-institutes:grid.6936.a
167 schema:familyName Rugel
168 schema:givenName G.
169 schema:sameAs https://app.dimensions.ai/discover/publication?and_facet_researcher=ur.0770662011.44
170 rdf:type schema:Person
171 sg:pub.10.1007/s004110050131 schema:sameAs https://app.dimensions.ai/details/publication/pub.1037305224
172 https://doi.org/10.1007/s004110050131
173 rdf:type schema:CreativeWork
174 grid-institutes:None schema:alternateName Maier-Leibnitz Laboratory, Faculty of Physics
175 schema:name Maier-Leibnitz Laboratory, Faculty of Physics
176 rdf:type schema:Organization
177 grid-institutes:grid.5252.0 schema:alternateName Radiobiological Institute, University of Munich, Schillerstrasse 42, 80336, Munich, Germany
178 schema:name Radiobiological Institute, University of Munich, Schillerstrasse 42, 80336, Munich, Germany
179 rdf:type schema:Organization
180 grid-institutes:grid.6936.a schema:alternateName Maier-Leibnitz Laboratory, Faculty of Physics, Technical University of Munich, 85747, Garching, Germany
181 schema:name Maier-Leibnitz Laboratory, Faculty of Physics, Technical University of Munich, 85747, Garching, Germany
182 Radiobiological Institute, University of Munich, Schillerstrasse 42, 80336, Munich, Germany
183 rdf:type schema:Organization
 




Preview window. Press ESC to close (or click here)


...