Long Range Plan for Nuclear Science: Building Blocks, Funding, and Collaboration

1. At this meeting two main issues: • Important building blocks of our long range plan: • Facilities with which to address the relevant key scientific questions in Nuclear science • Attract more EU fundings and strengthen the agreements and • collaboration programs with FA (via IA EU projects) • Messages and relevant inputs to pass to the working groups • (through the NuPECC liasons) • Examples: • This is a consolidating long range plan needed to express and comunicate in a coherent way the strong need to complete the major research infrastructures • Increase our visibility at Ministry level by adding our infrastructures in the ESFRI list • ……..

3. Planned Scheme (from the mail by the conveners) WG1 • Planning of the work in good shape • 1. Introduction • 2. Theoretical framework/progress • 3. Hadron Spectroscopy • subtopics: mesons, baryons, quarkonium, open flavor, exotics • Recent achievements/state of the art/open problems European perspective • Global perspective • 4.Hadron Structure • subtopics: Form factors, Parton distributions, TMDs, GPDs ... • Recent achievements/state of the art/open problems • European perspective Global perspective • 5. Hadronic interactions • subtopics: hyperon spin physics, hypernuclei ... • Recent achievements/state of the art/open problems European perspective • Global perspective • 6. Recommendations • 3.

5. WG2 - Properties of Strong-Interaction Matter • Weare preparing the first meeting of the Working Group 2, • whichwillhappenmostprobably on February 4. Weplan • to structure the work in the following way: • - in the first meeting (remote) weplan to have first discussions, • collectsuggestionsaboutwhateveryoneis ready to work on. • - FEB/MARCH 2016: next meeting to collect the input • from everybody and produce a skeleton of ourchapter (such • thatitbecomesvisiblewhat are the topicswewill deal with) • - APRIL/MAY 2016: produce a first version with contributions • from everybody (non-uniformdocument, butallsections in • place). A physical 1-2 days meeting may be usefulatthis stage. • SUMMER: completion and polishing of text

7. WG3 • Nuclear structure (Alexandre Obertelli) • with AB,AG,CD,ZD,BF,CF,MG,PG,SG,AJ,AK,NK,SL,AM,AO,NP,KR,AS,CS,CU • Nuclear reactions (Antonio Moro) with AK,AM,SS,CU • EoS investigation (Giuseppe Verde) with CF,MG,SL,NK,AS,CU,GV • Theory (Christian Forssen and Achim Schwenk) with CF,AG,AM,AS • Facilities and instrumentation (Stéphane Grevy) with SG,NK,SL,KR,CS,SS,CU,GV • WG3 members can belong to several subgroups, in order to facilitate discussion between the subgroups. The overlap with other NuPECC WG’s has also been raised, such as for instance nuclear structure for fundamental interactions. • The way the final WG3 document shall be written is left open • (introduction and chapters). For instance, it may be that once key • questions have emerged from subgroups, we could Schedule and actions : • ------------------------------ • February: a possible in person (or phone) meeting in ECT* could be organised for the whole WG3

9. Introduction (2 pages)aims and the links to other disciplines…… • 2. Physics – Origin of the Elements (10 pages) • Fingerprints of nucleosynthesis (1.5 pages) - Big Bang Nucleosynthesis (0.5 pages) • hydrostatic burning and s-process (2 pages) - Core collapse SN, p-process (1.5 pages) • Binary systems: novae, thermonuclear supernova, X-ray bursts (2 pages) • The matter of neutron stars (1 page) • The r-process (1 page) -Non-thermal nucleosynthesis (0.5 pages) • 3. Facilities and Tools (6 pages)(includes future requirements) • Experimental Facilities • Stable beam facilities (0.5 pages) • Radioactive beam facilities (1 page) • Underground facilities (0.5 pages) • Neutron measurements (0.5 pages) • Photonuclear measurements (0.5 pages) • AMS (0.5 pages) • Neutrino detectors (0.5 pages) • Nuclear Theory and Modelling (2 pages) • 4. Conclusions and Recommendations (2 pages)

11. Key issues to be addressed • Fundamental fermions • -Neutrino oscillations and the neutrino mixing matrix • - Neutrino masses (direct measurements and double β decay experiments) • -Quark mixing matrix and unitarity • -New (time reversal invariant) interactions in nuclear β decays and neutron decay • Discrete symmetries • -Parity violation • -Time reversal and CP violation in the quark sector (e.g. electric dipole moments) • -CPT and Lorentz invariance Nuclear Physics contributions to this physics

13. WG6 Meetings a ECT* Friday, March  4 Friday, July 8

14. Town meeting at GSI/FAIR NuPECC Long Range Plan Town Meeting, GSI Darmstadt, January 11-13, 2017 Invite our Observers A talk on the Long Range Plan in USA Invite the members of WG9 to attend? We need one or two editorial meetings among the coordinators of the NuPECC Liasons (myself and Sissy) One or two meetings between October and December 2016 One after the town meeting in January 2017

15. Spares

16. WG4 Meeting GSI KBW Lecture Hall on the 16th and 17th February 2016. https://indico.gsi.de/conferenceDisplay.py?confId=4402 We would like to collect inputs for the different working groups listed below. We invite you to send 2-3 slides with your physics suggestions to the working group leaders. The list of working groups is 1. Nuclear Theory for Nuclear Astrophysics (Stefan Typel, Nils Paar, Matthias Hempel) 2. Stable, gamma and neutron beams (Carlo Broggini, Rene Reifarth, Gyorgy Gyurky) 3. Radioactive beams (Cesar Domingo, Anu Kankainen, Nicolas de S?r?ville) 4. Stellar, supernova, and mergers models; chemical evolution (Raphael Hirschi, Friedrich R?pke?, Cristina Chiappini?) 5. Observations and data for nuclear astrophysics (Roland Diehl, Peter Hoppe?, Christof Vockenhuber)