INTERNATIONAL SCHOOL OF SUBNUCLEAR PHYSICS

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1 INTERNATIONAL SCHOOL OF SUBNUCLEAR PHYSICS WENNINGER The QGCW Project Quark-Gluon-Colored-World «ETTORE MAJORANA» FOUNDATION AND CENTRE FOR SCIENTIFIC CULTURE INTERNATIONAL SCHOOL OF SUBNUCLEAR PHYSICS STATUS OF THEORETICAL UNDERSTANDING AND OF EXPERIMENTAL POWER FOR LHC PHYSICS AND BEYOND 50TH ANNIVERSARY CELEBRATION OF THE QUARK WITH MURRAY GELL-MANN AND GEORGE ZWEIG ERICE: 24 JUNE 3 JULY 2014

2 How to study the New World

3 The QGCW Project (ABSTRACT extract ).. we propose to study the Quark Gluon Colored World (QGCW), which is totally different from our world made of QCD colorless baryons and mesons... The present Project is the first step. The next one being linked to the ELN collider with 300 km ring and total energy in PeV range..

4 INTERNATIONAL SCHOOL OF SUBNUCLEAR PHYSICS THE QGCW PROJECT: Technological Challenges to Study the New World «status report» INTERNATIONAL SCHOOL OF SUBNUCLEAR PHYSICS WHAT IS KNOWN AND UNEXPECTED AT LHC 48th Course, ERICE-SICILY: Directors: G. 'T HOOFT - A. ZICHICHI 29 AUGUST - 7 SEPTEMBER 2010

5 colliding nuclei: sheets of CGC? 0 fm 0.1 fm Glasma? growth of instabilities? transverse magnetic fields turbulance? Jets+ heavy quarks form jets are quenched, quarkonium screened, and flow develops time scale 1 fm 3x10-24 sec 1 fm QGP Phase sec 10 fm hadronization hadronic rescattering freezeout fm Courtesy: Paul Sorensen Highlightes from RHIC ERICE School 2008 detectors (meter) at detectors 10-9 sec (nanosecond)

6 Considering the time scales and evolution of the QCD matter produced in Heavy Ion collisions of order seconds we should start with probes produced together with the system they probe! jets and heavy quarkonia are QCD matter probes

7 but none-the-less development work is proposed at 2 levels to prepare the future Detectors Timing and synchronisation

8 (1) THE DETECTOR TECHNOLOGY The detector technology is under intense R&D since the synchronization needed is at a very high level of precision. The instruments must allow us to measure, as precisely as possible, the properties of all sub-nuclear particles coming out from the QGCW. THE MULTIGAP RESISTIVE PLATE CHAMBER MRPC the base of TOF

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10 Timing and beam synchronization The Large Hadron Collider uses a technology to synchronize systems within 10 nanoseconds. With an oscillator-based master clock, CERN can supply its equipment with time data with an accuracy of one nanosecond. The fieldbus used to network a large number of systems together is linked to a GPS system. The data from that system is relayed to equipment across the Large Hadron Collider to keep everything synchronized to universal time. One of the most challenging tasks is keeping 1,800 power converters synchronized to within one millisecond. It also serves to synchronize radiation monitoring, magnet alignment, and other systems at the LHC. The common timing and trigger distribution system developed at CERN is also used by the four experiments.

11 since 2010 the results from RHIC and LHC heavy ion experiments have shown many interesting properties of the QGCW The important contribution to the results obtained with instruments such as the LAA - MRPC the base of Bologna TOF which allowed to measure precisely the properties of all sub-nuclear particles coming out from the QGCW in ALICE is shown in the following slides by Roberto Preghenella from the Centro Fermi Roma

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18 The Large Hadron Collider uses a technology to synchronize systems within 10 nanoseconds. The fieldbus used to network a large number of systems together is linked to a GPS system. The data from that system is relayed to equipment across the Large Hadron Collider to keep everything synchronized to universal time. With an oscillator-based master clock, CERN can supply its equipment with time data with an accuracy of one nanosecond. Advanced R&D has started also for FAIR at GSI. The Bunch-phase Timing System (BuTiS) for FAIR concentrates on the research of thermal stability properties of optical fibres. The work is done by the communications institute of TU Darmstadt under contract with GSI. The term bunch phase shall emphasize the kind of timing precision that is dealt with in the system

19 INTERNATIONAL SCHOOL OF SUBNUCLEAR PHYSICS WENNINGER The QGCW Project interesting new opportunities for young talents FAIR - Facility for Antiproton and Ion Research overview of R&D for FAIR detectors and accelerator systems «ETTORE MAJORANA» FOUNDATION AND CENTRE FOR SCIENTIFIC CULTURE INTERNATIONAL SCHOOL OF SUBNUCLEAR PHYSICS STATUS OF THEORETICAL UNDERSTANDING AND OF EXPERIMENTAL POWER FOR LHC PHYSICS AND BEYOND 50TH ANNIVERSARY CELEBRATION OF THE QUARK WITH MURRAY GELL-MANN AND GEORGE ZWEIG ERICE: 24 JUNE 3 JULY 2014

20 FAIR Science Overview courtesy: Boris Sharkov, Inti Lehmann et al. Atomic, applied and plasma physics - APPA Hadron structure - PANDA big bang time QCD phase transition - CBM temperature Astrophysics and nuclear structure - NUSTAR

21 CBM Physics Case RHIC, LHC FAIR Courtesy of T. Hatsuda The equation-of-state at high baryonic density New phases of stronglyinteracting matter Deconfinement phase transition at high baryonic density QCD critical endpoint Onset of chiral symmetry restoration at high baryonic density Strange matter

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23 Experimental sides at UNILAC material science applications plasma physics PHELIX SHIP/SHIPTRAP TASCA biophysics nuclear physics 7/1/2014

24 Experimental sides at SIS18/ESR Production target nuclear physics hadron physics Synchrotron Accelerator U ions up to 1 GeV/u Separation detector setup implantation g-spectroscopy Storage ring with detectors biophysics atomic physics HADES Erice 2014

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26 The FAIR Project APPA ions, antiprotons CBM relativistic nuclear collisions PANDA antiproton beams NUSTAR radioactive ion beams

27 This year also UK ( Associate Member )

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29 FAIR India Research Center has meanwhile been set up as well

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33 APPA Physics (Atomic, Plasma Physics and Applications) BIOMAT (Biology and Material Science) FLAIR (Facility for Low-Energy Antiproton and Heavy Ion Research) HEDgeHOB (High Energy Density Matter generated by Heavy Ion Beams) SPARC (Stored Particles Atomic Research Collaboration) WDM (Warm Dense Matter) collaboration Nuclear Matter Physics CBM (Compressed Baryonic Matter) experiment NUSTAR Physics (Nuclear Structure, Astrophysics and Reactions) MATS DESPEC/HISPEC (Decay Spectroscopy/High-Resolution Spectroscopy) ELISe (Electron-Ion Scattering in a Storage Ring) EXL (Exotic nuclei studied in light-ion induced reactions at the NESR) ILIMA (Isomeric Beams, Lifetimes and Masses) LaSpec (Laser Spectroscopy) (Precision Measurements of very short-lived nuclei with Advanced Trapping) R3B (Reactions with Relativistic Radioactive Beams) SuperFRS (Super Fragment Separator) project Physics with High Energy Antiprotons PANDA (Antiproton Annihilation at Darmstadt) experiment

34 Primary Beams Facility for Antiproton and Ion Research new accelerator challenges and R&D /s; 1.5 GeV/u; 238 U /s 238 U 73+ up to 35 GeV/u 3x10 13 /s 30 GeV protons Secondary Beams p-linac SIS18 Technical Challenges cooled beams, rapid cycling SIS100/300 superconducting magnets range of radioactive beams up to GeV/u; up to factor higher in intensity than presently antiprotons 3-30 GeV Storage and Cooler Rings HESR Rare-Isotope Production Target Anti-Proton Production Target radioactive beams antiprotons GeV/c, stored and cooled CR & RESR 100 m NESR Cryring

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36 APPA APPA Atomic, Plasma Physics and Applications About 700 members Wide field of science basic research to material, biological and medical applications Atomic Physics SPARC: 284 members from 26 countries FLAIR: 144 members from 15 countries Plasma Physics HEDgeHOB & WDM: 175 members from 16 countries Materials Research and Biophysics BIOMAT: 110 members from 12 countries

37 Temperature [ev] APPA: Plasma Physics Reach Magnetic Fusion Inertial Fusion Energy Laser Heating PHELIX XFEL FLASH SIS 100 Sun Core Sun Surface Ion Beam Heating SIS 18 solid state density Jupiter Particles / cm -3

38 APPA: Biology / Medicine Biological effects of heavy ions crucial for manned space exploratio ns Adenoid cystic carcionom 12 C GSI NASA and ESA engaged

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40 CBM CBM Compressed Baryonic Matter About 400 members

41 Muon Tracking Ring Imaging Cherenkov Detector Transition Radiation Detectors CBM Detector Electromagnetic Calorimeter Silicon Tracking Stations Vertex Detector Projectile Spectator Detector (Calorimeter) Dipol magnet Resistive Plate Chambers (TOF)

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46 NUSTAR Super- FRS Nuclear Structure, Astrophysics and Reactions About 800 members NUSTAR

47 NUSTAR Physics Case Nuclear structure Underlying QCD structure complex nucleon-nucleon force Study of exotic short lived nuclei far off stability (proton/ neutron skins or halos, new magic numbers...) Pave way for theoretical framework with predictive power for nuclei beyond experimental reach Astrophysics Origin of the heavy elements? Physics of stellar explosions (core-collapse, thermonuclear supernovae, nucleosynthesis) Compact objects and the explosions on their surfaces (x-ray bursts) 7/1/2014 Erice 2014

48 NUSTAR Production of intensive rare isotope beams by in-flight projectile fragmentation/fission (access to short-lived isotopes) Detailed investigations, large variety of experimental techniques 7/1/2014 Erice 2014

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50 PANDA Antiproton Annihilations at Darmstadt About 500 members PANDA

51 PANDA Physics Case Gluonic excitations Hybrids, glueballs Charmonium states Precision spectroscopy Time-like Form factors, nucleon structure In medium mass modifications Extension to the charm sector Extension of nuclear chart Double hypernuclei And much more... p K D p - p + K + D - 50 MeV D + 25 MeV 100 MeV K -

52 PANDA Energy Range

53 PANDA Experimental Set-Up Fixed target magnetic spectrometer experiment Target Spectrometer Forward Spectrometer Beam Dipole Solenoid Interaction point

54 Collaboration Members by Country

55 Modularised Start Version M0 Cost about 1.6 billion by 2018 (1 billion 2005 Euros) M3 M1 M3 M2 CBM/HADES Modules M0: SIS100 M1: APPA M1: CBM/HADES M2: NUSTAR M3: PANDA PANDA APPA NUSTAR

56 Well progressing Accelerator s Progress SIS 100 dipoles First series del.+tested SIS 100 sextopoles Dubna prototype HEBT magnets Efremov, St Petersburg SIS 100 quadrupoles JINR, Dubna

57 Roadmap Experiments

58 Experiments Progress Science review Scientific Council s 2 nd meeting Very positive outcome Technical evaluation Expert Committee Experiments 3 very efficient meetings, 4 th meeting in June members (extended from 9) 21 TDRs submitted, 14 approved Funding 60% secured, 20% EoIs, partners sought for 20% Resources Review Boards established 2 very efficient meetings, 3 rd in June st Collaboration Contract drafted

59 Licensing Applications / Permits General construction permit for all buildings by city of Darmstadt: Oct 2012

60 Funding 526 M for civil construction largest BMBF grant ever

61 FAIR Civil Construction: Status 2010 to /1/2014? Erice

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63 OPENING LECTURE ANTONINO ZICHICHI We should be prepared with powerful experimental instruments, technologically at the frontier of our knowledge to discover Totally Unexpected Events

64 Thank you