PPT-1 Front End for MAP Neutrino Factory

Collider rf considerations David Neuffer May 2014 2 Outline Previous baseline was 200 MHz IDS nu Factory Rf power req Front End for MAP NFMC 325 MHz Bunch train shorter than IDS . Oscillations. Collective Neutrino Oscillations. Georg G. Raffelt. 3. rd. Schr. ödinger Lecture, Thursday 19 May 2011. Neutrino Oscillations in Matter. 3300 citations. Lincoln Wolfenstein. Neutrinos in a medium suffer . Satoshi Nakamura. Osaka University, Japan. Collaborators : H. . Kamano. (RCNP, Osaka Univ.), T. Sato (Osaka Univ.). T.-S.H. Lee (Argonne Nat’l Lab). Contents. Introduction . 1. May, 5th 2015. Vertical/. Floor. . big. . beams. . connection. with. an angle . stiffener. Neutrino. 2. May, 5th 2015. Vertical/. Floor. . big. . beams. . connection. with. an angle . stiffener. COSMOLOGY. EVIDENCE FOR NEW PHYSICS?. STEEN . HANNESTAD, Aarhus . University. NuHorizons. 2011. n. e. n. m. n. t. Fermion Mass Spectrum. 10. 100. 1. 10. 100. 1. 10. 100. 1. 10. 100. 1. Alan Bross. N u F a c t 0 9. From . SuperBeams. to Neutrino Factories. Pre-Ramble. Neutrino Factory means different things to different people. Not so much for . SuperBeams. I will be talking about a muon-based Neutrino Factory as opposed to a . . . Neutrinos Are Very Elusive!. We now understand that neutrinos are produced in nuclear reactions, but they were actually . predicted several decades before they were finally discovered. . O. n what basis was that prediction made?. Art McDonald, Professor Emeritus. Queen’s University, Kingston, . Ontario, Canada. T. he middle of the sun is so hot that the centers of the atoms (nuclei). f. use together, giving off lots of energy and neutrinos. The neutrinos penetrate easily through the dense material in the Sun and reach the earth.. -chicane & absorber. David . Neuffer. C. Rogers, P. . Snopok. , C. Yoshikawa, …. 2012. 2. Outline. Front End for the IDS Neutrino Factory. Basis for engineering/costs. Rf. , requirements . Engineering required. -chicane & absorber. David . Neuffer. C. Rogers, P. . Snopok. , C. Yoshikawa, …. 2012. 2. Outline. Front End for the IDS Neutrino Factory. Basis for engineering/costs. Rf. , requirements . Engineering required. End. (IPAC13, TUPFI075. ) . H. K. Sayed,. *1. . J.S. Berg. 1. , X. Ding. 2. , . H.G Kirk,. 1. . K.T. McDonald. 3. 1 . Brookhaven National Laboratory, Upton, NY 11953, USA. 2. UCLA, Los Angeles, CA 90095, USA. Are we close to measuring the neutrino hierarchy? Filipe B. Abdalla ν Loureiro , Moraes , Abdalla et al. arXiv:1809.07204 Loureiro , Cuceu , Abdalla et al. arXiv:1811.02578 Outline Cosmology background Mandate. “Rapid progress in neutrino oscillation physics, with significant European involvement, has established a strong scientific case for a long-baseline neutrino programme exploring CP violation and the mass hierarchy in the neutrino sector. CERN should develop a neutrino program to . Chicane update. David . Neuffer. February 12, . 2013. 2. Outline. Front End for the IDS Neutrino Factory. Losses . – control. Chicane, proton . absorber. rematching. OK. Re-Match includes chicane + absorber. http://www.darkenergysurvey.org. . . . Outline. DES: what is it and update + probes used. Dark energy from DES.. Neutrino masses from DES. Filipe . Batoni. . Abdalla. Future Dark Energy Surveys.