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zadetkov: 75
1.
  • Alignment methods for the O... Alignment methods for the OPERA drift tube detector
    Büttner, B.; Ebert, J.; Ferber, T. ... Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment, 05/2014, Letnik: 747
    Journal Article
    Recenzirano

    The goal of the OPERA experiment is to give the first direct evidence for neutrino oscillations in the channel νμ→ντ. The OPERA detector is designed to observe the appearance of tau neutrinos in the ...
Celotno besedilo
2.
  • Search for $\nu_\mu \righta... Search for $\nu_\mu \rightarrow \nu_e$ oscillations with the OPERA experiment in the CNGS beam
    Agafonova, N.; Aleksandrov, Alexander; Anokhina, A. ... The journal of high energy physics, 2013, Letnik: 7(2013)
    Journal Article
    Recenzirano

    A first result of the search for \numu $\rightarrow$ \nue oscillations in the OPERA experiment, located at the Gran Sasso Underground Laboratory, is presented. The experiment looked for the ...
Celotno besedilo

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3.
  • The gas system of the drift... The gas system of the drift tube detector of the neutrino experiment OPERA
    Ferber, T.; Bick, D.; Ebert, J. ... Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment, 07/2008, Letnik: 592, Številka: 3
    Journal Article
    Recenzirano

    The gas system of the drift tube detector of the neutrino experiment OPERA is presented. The drift tube detector, called precision tracker (PT), consists of 10 000 thinwalled aluminum tubes of 38 mm ...
Celotno besedilo
4.
  • Search for $\nu_\mu\rightar... Search for $\nu_\mu\rightarrow\nu_\tau$ oscillation with the OPERA experiment in the CNGS beam
    Agafonova, N.; Aleksandrov, Alexander; Altinok, O. ... New journal of physics, 2012, Letnik: 14
    Journal Article
    Recenzirano

    The OPERA neutrino experiment in the underground Gran Sasso Laboratory (LNGS) was designed to perform the first detection of neutrino oscillations in direct appearance mode in the ...
Celotno besedilo

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5.
  • Observation of a first $\nu... Observation of a first $\nu_\tau$ candidate in the OPERA experiment in the CNGS beam
    Agafonov, N.; Aleksandrov, Alexander; Altinok, O. ... Physics letters. B, 2010, Letnik: 691
    Journal Article
    Recenzirano

    The OPERA neutrino detector in the underground Gran Sasso Laboratory (LNGS) has been designed to perform the first detection of neutrino oscillations in direct appearance mode through the study of ...
Celotno besedilo

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6.
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7.
  • New results on [nu]^sub [mu]^ [arrow right] [nu]^sub [tau]^ appearance with the OPERA experiment in the CNGS beam
    Aleksandrov, A; Anokhina, A; Aoki, S ... The journal of high energy physics, 11/2013, Letnik: 2013, Številka: 11
    Journal Article
    Recenzirano
    Odprti dostop

    The OPERA neutrino experiment is designed to perform the first observation of neutrino oscillations in direct appearance mode in the nu ^sub mu^ arrow right nu ^sub tau^ channel, via the detection of ...
Celotno besedilo

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8.
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9.
  • Search for [nu]^sub [mu]^ [arrow right] [nu]^sub e^ oscillations with the OPERA experiment in the CNGS beam
    Aleksandrov, A; Anokhina, A; Ariga, A ... The journal of high energy physics, 07/2013, Letnik: 2013, Številka: 7
    Journal Article
    Recenzirano
    Odprti dostop

    (ProQuest: ... denotes formulae and/or non-USASCII text omitted; see image) A first result of the search for nu ^sub mu^ arrow right nu ^sub e^ oscillations in the OPERA experiment, located at the ...
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10.
  • Application of Finite Eleme... Application of Finite Element Analysis to Helmet Design
    Smith, Terry; Lenkeit, John; Boughton, Jim IUTAM Symposium on Impact Biomechanics: From Fundamental Insights to Applications
    Book Chapter
    Recenzirano

    This paper describes an alternative method for helmet design using finite element analysis (FEA). While previous research has illustrated the use of FEA as a tool to simulate standard helmet tests, ...
Celotno besedilo
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zadetkov: 75

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