The Long-Baseline Neutrino Experiment: Exploring Fundamental Symmetries of the Universe
By LB Adams, D. Adams, T. Akiri, T. Alion, K. Anderson, C. Andreopoulos, M. Andrews, I. Anghel, J. Anjos, M. Antonello and 557 more. 2013
318 citations recorded by the source corpus.
The preponderance of matter over antimatter in the early Universe, the dynamics of the supernova bursts that produced the heavy elements necessary for life and whether protons eventually decay --- these mysteries at the forefront of particle physics and astrophysics are key to understanding the early evolution of our Universe, its current state and its eventual fate. The Long-Baseline Neutrino Experiment (LBNE) represents an extensively developed plan for a world-class experiment dedicated to addressing these questions. LBNE is conceived around three central components: (1) a new, high-intensity neutrino source generated from a megawatt-class proton accelerator at Fermi National Accelerator Laboratory, (2) a near neutrino detector just downstream of the source, and (3) a massive liquid argon time-projection chamber deployed as a far detector deep underground at the Sanford Underground Research Facility. This facility, located at the site of the former Homestake Mine in Lead, South Dakota, is approximately 1,300 km from the neutrino source at Fermilab -- a distance (baseline) that delivers optimal sensitivity to neutrino charge-parity symmetry violation and mass ordering effects. This ambitious yet cost-effective design incorporates scalability and flexibility and can accommodate a variety of upgrades and contributions. With its exceptional combination of experimental configuration, technical capabilities, and potential for transformative discoveries, LBNE promises to be a vital facility for the field of particle physics worldwide, providing physicists from around the globe with opportunities to collaborate in a twenty to thirty year program of exciting science. In this document we provide a comprehensive overview of LBNE's scientific objectives, its place in the landscape of neutrino physics worldwide, the technologies it will incorporate and the capabilities it will possess.
View Paper: https://www.semanticscholar.org/paper/0975b5b087e6378ee8696662590ef3acef3c08d8
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Citations in the corpus
- On the description of nonunitary neutrino mixing (2015, methodology): “Future experimental proposals, such as DUNE [64] and ILC, expect to improve these constraints [65] In Fig.”
- Heavy Neutral Leptons at FASER (2018, background): “This region in the parameter space for both electron and muon mixing will also be probed by the future DUNE facility for which we show results following [47].”
- Long-Baseline Neutrino Facility (LBNF) and Deep Underground Neutrino Experiment (DUNE) Conceptual Design Report Volume 1: The LBNF and DUNE Projects (2015, methodology): “And conversely, conducting precision measurements of neutrino interactions will actually result in a reduction of systematic uncertainties on signal and background predictions in the far detector [183, 184, 19].”
- Long-Baseline Neutrino Facility (LBNF) and Deep Underground Neutrino Experiment (DUNE) Conceptual Design Report Volume 2: The Physics Program for DUNE at LBNF (2015, methodology): “The fast Monte Carlo tool is based on work done for the far detector[47] (Appendix A.”
- KM3MeT 2.0 Letter of intent for ARCA and ORCA (2016, background): “The νe appearance channel is the main focus of current (such as NOvA [104] and T2K [105]) and next-generation (such as CHIPS [106], LBNE [107], LBNO [108] or more recently DUNE [109]) accelerator neutrino experiments.”
- Physics beyond colliders at CERN: beyond the Standard Model working group report (2019, background): “30 m and assuming a normal hierarchy of neutrinos masses [295] and from FCC-ee with 10(12) Z decays and HNLs decaying between 10 and 100 cm from the interaction vertex [296].”
- A facility to Search for Hidden Particles (SHiP) at the CERN SPS (2015, background): “A case study for an HNL search has been performed [235], ignoring all backgrounds.”