Open Access
EPJ Web Conf.
Volume 234, 2020
International Workshop on “Flavour Changing and Conserving Processes” (FCCP2019)
Article Number 01003
Number of page(s) 6
Published online 27 April 2020
  1. M. Anelli et al., A facility to Search for Hidden Particles (SHiP) at the CERN SPS, arXiv:1504.04956. [Google Scholar]
  2. S. Alekhin et al., A facility to search for hidden particles at the CERN SPS: the SHiP physics case, Rep. Prog. Phys. 79 (2016) 124201. [Google Scholar]
  3. A. Akmete et al., The active muon shield in the SHiP experiment, JINST 12 (2017) no.05, P05011. [Google Scholar]
  4. C. Ahdida et al., The experimental facility for the Search for Hidden Particles at the CERN SPS, JINST 14 (2019) no.03, P03025. [Google Scholar]
  5. C. Ahdida et al., The Magnet of the Scattering and Neutrino Detector for the SHiP experiment at CERN, arXiv:1910.02952. [Google Scholar]
  6. N. Agafonova et al., The OPERA experiment in the CERN to Gran Sasso neutrino beam, JINST 4 (2009) P04018. [Google Scholar]
  7. C. Fukushima et al., A thin emulsion spectrometer using a compact permanent magnet, Nucl. Instrum. Meth. A592 (2008) 56. [Google Scholar]
  8. E. Cerron Zeballos et al., A New type of resistive plate chamber: The Multigap RPC, NIMA 374 (1996) 132-135. [Google Scholar]
  9. C. Ahdida et al., Sensitivity of the SHiP experiment to Heavy Neutral Leptons, JHEP 1904 (2019) 077. [Google Scholar]
  10. K. Kodama et al., Final tau-neutrino results from the DONuT experiment, Phys. Rev. D78 (2008) 052002. [Google Scholar]
  11. N. Agafonova et al., Observation of a first ντ candidate in the OPERA experiment in the CNGS beam, Phys. Lett. B691 (2010) 138. [Google Scholar]
  12. N. Agafonova et al., New results on νµ ντ appearance with the OPERA experiment in the CNGS beam, JHEP 1311 (2013) 036. [Google Scholar]
  13. N. Agafonova et al., Evidence for νµ ντ appearance in the CNGS neutrino beam with the OPERA experiment, Phys. Rev. D89 (2014) 051102. [Google Scholar]
  14. N. Agafonova et al., Observation of tau neutrino appearance in the CNGS beam with the OPERA experiment, PTEP 2014 (2014) 101C01. [Google Scholar]
  15. N. Agafonova et al., Discovery of τ neutrino appearance in the CNGS Neutrino Beam with the OPERA experiment, Phys. Rev. Lett. 115 (2015) 121802. [Google Scholar]
  16. N. Agafonova et al., Final results of the OPERA experiment on ντ appearance in the CNGS beam, Phys. Rev. Lett. 120 (2018) 211801. [Google Scholar]
  17. G. De Lellis et al., Charm physics with neutrinos, Physics Reports 399 (2004) 227. [CrossRef] [Google Scholar]
  18. T. Adams et al., Evidence for diffractive charm production in muon-neutrino Fe and anti-muon-neutrino Fe scattering at the Tevatron, Phys.Rev. D61 (2000) 092001 [Google Scholar]
  19. A. Kayis-Topaksu et al., Measurement of charm production in neutrino charged-current interactions, New J.Phys. 13 (2011) 093002. [CrossRef] [Google Scholar]
  20. G. Onengut et al., Measurement of charm production in antineutrino charged-current interactions, Phys.Lett. B604 (2004) 11-21. [CrossRef] [Google Scholar]
  21. H. Dijkstra and T. Ruf, [Google Scholar]
  22. C. Lourenco, H.K. Wohri, Heavy flavour hadroproduction from fixed-target to collider energies, Physics Reports 433 (2006) 127. [Google Scholar]
  23. A. Akmete et al., Measurement of associated charm production induced by 400 GeV/c protons, CERNSPSC-2017-033, SPSC-EOI-017 (2017). [Google Scholar]
  24. F. Hugging, The ATLAS Pixel Insertable B-Layer (IBL), Nucl. Instrum. Meth., A650 (2011) 45–49. [CrossRef] [Google Scholar]
  25. M. Garcia-Sciveres et al., The FE-I4 pixel readout integrated circuit, Nucl. Instrum. Meth. A636 (2011) S155–S159. [CrossRef] [Google Scholar]
  26. R. Zimmermann et al., The precision tracker of the OPERA detector, Nucl. Instrum. Meth., A555 (2005) 435–450. [CrossRef] [Google Scholar]
  27. S. Petrera and G. Romano, A method to evaluate the detection efficiency and the mean lifetime of shortlived particles, Nucl. Instrum. Meth. 174 (1980) 61. [CrossRef] [Google Scholar]
  28. CTEQ collaboration, Handbook of perturbative QCD: Version 1.0, Rev. Mod. Phys. 67 (1995) 157. [Google Scholar]
  29. J. M. Conrad, M. H. Shaevitz and T. Bolton, Precision measurements with high-energy neutrino beams, Rev. Mod. Phys. 70 (1998) 1341. [Google Scholar]
  30. J. A. Formaggio and G. P. Zeller, From eV to EeV: Neutrino Cross Sections Across Energy Scales, Rev. Mod. Phys. 84 (2012) 1307. [Google Scholar]
  31. A. Connolly, R. S. Thorne and D. Waters, Calculation of High Energy Neutrino-Nucleon Cross Sections and Uncertainties Using the MSTW Parton Distribution Functions and Implications for Future Experiments, Phys. Rev. D83 (2011) 113009. [Google Scholar]
  32. C.-Y. Chen, P. S. Bhupal Dev and A. Soni, Standard model explanation of the ultrahigh energy neutrino events at IceCube, Phys. Rev. D89 (2014) 033012. [Google Scholar]
  33. D. Marfatia, D. W. McKay and T. J. Weiler, New physics with ultra-high-energy neutrinos, Phys. Lett. B748 (2015) 113. [CrossRef] [Google Scholar]
  34. M. Ackermann et al., Astrophysics Uniquely Enabled by Observations of High-Energy Cosmic Neutrinos, Bull. Am. Astron. Soc. 51 (2019) 185. [Google Scholar]
  35. IceCube collaboration, Measurement of the multiTeV neutrino cross section with IceCube using Earth absorption, Nature 551 (2017) 596. [Google Scholar]
  36. M. Bustamante and A. Connolly, Extracting the Energy-Dependent Neutrino-Nucleon Cross Section above 10 TeV Using IceCube Showers, Phys. Rev. Lett. 122 (2019) 041101. [CrossRef] [PubMed] [Google Scholar]
  37. N. Beni et al., Physics Potential of an Experiment using LHC Neutrinos, J. Phys. G46 (2019) 115008. [Google Scholar]
  38. C. Ahdida et al., SND@LHC, CERN-LHCC-2020002, LHCC-I-035. [Google Scholar]

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.