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008 | 170212s2015 gw | s |||| 0|eng d | ||
020 |
_a9783319185279 _9978-3-319-18527-9 |
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024 | 7 |
_a10.1007/978-3-319-18527-9 _2doi |
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035 | _ato000559849 | ||
040 |
_aSpringer _cSpringer _dRU-ToGU |
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_aPHP _2bicssc |
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_aSCI051000 _2bisacsh |
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082 | 0 | 4 |
_a539.73 _223 |
100 | 1 |
_aKluck, Holger. _eauthor. _9466339 |
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245 | 1 | 0 |
_aProduction Yield of Muon-Induced Neutrons in Lead _helectronic resource _bMeasured at the Modane Underground Laboratory / _cby Holger Kluck. |
250 | _a1st ed. 2015. | ||
260 |
_aCham : _bSpringer International Publishing : _bImprint: Springer, _c2015. |
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300 |
_aXXV, 382 p. 91 illus., 65 illus. in color. _bonline resource. |
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336 |
_atext _btxt _2rdacontent |
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337 |
_acomputer _bc _2rdamedia |
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338 |
_aonline resource _bcr _2rdacarrier |
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490 | 1 |
_aSpringer Theses, Recognizing Outstanding Ph.D. Research, _x2190-5053 |
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505 | 0 | _aIntroduction -- Edelweiss: Direct Dark Matter Search at LSM -- Review of Muon-Induced Neutron Production at Underground Sites -- Long Term Measurement of Muon-induced Neutrons at LSM -- Assessment of Geant4 to Simulate the Neutron Yield in Lead at LSM -- Conclusion and Outlook -- Appendix. | |
520 | _aThe work presented in this book is a major step towards understanding and eventually suppressing background in the direct search for dark matter particles scattering off germanium detectors. Although the flux of cosmic muons is reduced by many orders of magnitude in underground laboratories, the remaining energetic muons induce neutrons through various processes, neutrons that can potentially mimic a dark matter signal.This thesis describes the measurement of muon-induced neutrons over more than 3 years in the Modane underground laboratory. The data are complemented by a thorough modeling of the neutron signal using the GEANT4 simulation package, demonstrating the appropriateness of this tool to model these rare processes. As a result, a precise neutron production yield can be presented. Thus, future underground experiments will be able to reliably model the expected rate of muon-induced neutrons, making it possible to develop the necessary shielding concept to suppress this background component. | ||
650 | 0 |
_aphysics. _9566227 |
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650 | 0 |
_aastronomy. _9191712 |
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650 | 0 |
_aAstrophysics. _9303267 |
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650 | 0 |
_aCosmology. _9410497 |
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650 | 0 |
_aParticle acceleration. _9305194 |
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650 | 0 |
_aPhysical measurements. _9461481 |
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650 | 0 |
_aMeasurement. _9461482 |
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650 | 1 | 4 |
_aPhysics. _9566228 |
650 | 2 | 4 |
_aParticle Acceleration and Detection, Beam Physics. _9305195 |
650 | 2 | 4 |
_aAstronomy, Astrophysics and Cosmology. _9566245 |
650 | 2 | 4 |
_aMeasurement Science and Instrumentation. _9143946 |
710 | 2 |
_aSpringerLink (Online service) _9143950 |
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773 | 0 | _tSpringer eBooks | |
830 | 0 |
_aSpringer Theses, Recognizing Outstanding Ph.D. Research, _9567110 |
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856 | 4 | 0 | _uhttp://dx.doi.org/10.1007/978-3-319-18527-9 |
912 | _aZDB-2-PHA | ||
999 | _c414487 |