PPT-1 Proton vs neutron EDM in general MSSM

Diego Mart í nez Santos Miriam Lucio Isabel Suarez 2 Motivation Disclaimer Im an experimentalist Try to address the following questions Can be NP very different in d p and . precision measurements: what do they provide?. precision experiments part of large facilities. precision experiments with neutrons. Precision experiments. Electroweak precision experiments. proton decay measurements. Misak Sargsian. Florida International University, Miami. Hadrons in the . Nuclear. Medium. CLAS 12 2. nd. European Workshop. 7-11, March 2010, Paris. High Energy Electro- Nuclear Processes . Elemental humor. Explain the science behind this:. A proton, neutron, and electron went out to dinner one night.  After a luxurious meal, the waiter brought . their checks . to the proton and the electron.  The neutron was perplexed as to why the waiter didn't bring him his check.  So, he summoned the waiter to the table and asked him about it.. Saturday Physics for Everyone. November 9, 2013. (With debts to Chris Quigg, Leonard Susskind, Hitoshi Murayama). Why is there mass?. What . is mass?. Mass is . stuff. Mass is the . stuff. that gravity acts on. Mikhail E. . Gusakov. , . Vasiliy. A. . Dommes. Ioffe. Institute. Saint-Petersburg, Russia. Introduction. . It is generally accepted that baryons (neutrons and protons) in the internal layers of neutron stars undergo transition into superfluid/superconducting state at .. for high power deuterium beams. Corso di Dottorato in Fisica e Astronomia: ciclo XXX. Seminario di fine primo anno. Andrea . Muraro. Outline. What is ITER . Neutral Beam Injector for ITER (PRIMA). CNESM Principle. Pacific Northwest National Laboratory. February 18, 2015. 1. MCNP – What Is It?. Monte Carlo particle transport code merging MCNP (<20 MeV for neutrons) and LAHET tracking high energy particles. Neutron number (N). Proton number (Z). University of York. (Replace with institution name) . Nuclear physics in stars. The CNO cycle – catalysts for stars. HotCNO. . Where do heavy elements come from?. EDMs and BSM (Beyond Standard Model) physics. New CP violation - . Baryogenesis. ?. How to identify origin of new CP violation. Need data from multiple species. Summary of . experiments. Short overview. bomlása során . 90. Th. 234. thórium . . keletkezik. A reakció másik terméke.... A) hidrogénizotóp (proton)_____. 1. H. 1. B) hidrogénizotóp (deutérium)__. 1. H. 2. C) héliumizotóp______________. Part I. . Unstable. vs. . stable. nuclei: . neutron-rich. and . proton-rich. . systems. Limit of . nuclear. . stability. and . definition. of . drip. . lines. From: Exotic Nuclei, J. Enders, TU Darmstadt, Summer 2003. . 1. Important questions. .  . B. . What observables are sensitive to the EOS and at what densities. ?. 0. Astrophysical observables (neutron stars). . . 1. Binding energies . . 2. Radii of neutron and proton matter in nuclei . W. . Reviol, D. Rudolph, D.G. Sarantites, . C.J. Chiara. , D. . . Seweryniak. Washington . U. / Lund U. / U. of Maryland / ANL. Gretina Workshop, . ANL, . March . 2013. Neutron-Shell . Detectors. 35 hexagonal, tapered detectors.. Paul Mantica. Lecture 1. Euroschool. for Exotic Beams. Leuven, Belgium - 2009. Beta . Decay . of . Exotic Nuclei:. Science . Opportunities. Gamow-Teller strength in N~Z nuclei to . 100. Sn. Persistence of shell gaps in extreme neutron-rich nuclei (.