Topology of “ white ” stars in relativistic fragmentation of

Slides:

Advertisements

Similar presentations

Neutron detectors and spectrometers 1) Complicated reactions → strong dependency of efficiency on energy 2) Small efficiency → necessity of large volumes.

Advertisements

Ion Beam Analysis techniques:

1 General characteristics of AA collisions at 35 AGeV Yuri Kharlov, Serguei Sadovsky IHEP, Protvino LINC-2005, 5 October 2005.

The peculiarities of the production and decay of superheavy nuclei M.G.Itkis Flerov Laboratory of Nuclear Reactions, JINR, Dubna, Russia.

11 Study of light nuclei cluster structure with nuclear track emulsion Denis Artemenkov, VBLHEP, JINR Predeal-Romania October 14-18, 2013.

Results from PHENIX on deuteron and anti- deuteron production in Au+Au collisions at RHIC Joakim Nystrand University of Bergen for the PHENIX Collaboration.

Bucharest emulsion group along the time Who we are.

Brief History of Nuclear Physics 1896-Henri Becquerel ( ) discovered radioactivity 1911-Ernest Rutherford ( ), Hanz Geiger ( )

Nucleus. Nuclear Notation  The nucleus consists of protons and neutrons. Protons: Z (atomic number) Neutrons: N Nucleons: A = Z + N (atomic mass) Full.

Analysis of Light Single-  Hypernuclei Events in Nuclear Emulsion Detected with Overall-scanning Method MYINT KYAW SOE, Kazuma NAKAZAWA, Kaoru HOSHINO,

11 Study of light nuclei cluster structure with nuclear track emulsion Denis Artemenkov VBLHEP, JINR EFB22-Krakow-2013.

N. Saito The RISING stopped beam physics meeting Technical status of RISING at GSI N. Saito - GSI for the RISING collaboration Introduction Detector performance.

C-REX (little sister of PREX) : Parity-Violating Measurement of the Weak Charge radius of 48 Ca to 0.03 fm. 1-pass (2.2 GeV) HRS + septum C-REX Workshop.

Applications of neutron spectrometry Neutron sources: 1) Reactors 2) Usage of reactions 3) Spallation sources Neutron show: 1) Where atoms are (structure)

Isotopically resolved residues produced in the fragmentation of 136 Xe and 124 Xe projectiles Daniela Henzlova GSI-Darmstadt, Germany on leave from NPI.

23 July 2010FLNR Dubna Summer Students Practice Flerov Laboratory of Nuclear Reactions, JINR, Dubna 2010 JINR, Dubna 2010 Studies with radioactive ion.

Topology of multifragmentation of light relativistic nuclei by P. I. Zarubin, JINR On behalf of the BECQUEREL Collaboration All this and more on the Web.

106 th Session of the JINR Scientific Council September 24-25, 2009, Dubna Perspectives of JINR – ORNL Collaboration in the Studies of Superheavy Elements.

XVIII International Baldin Seminar on High Energy Physics Problems "RELATIVISTIC NUCLEAR PHYSICS & QUANTUM CHROMODYNAMICS“ Dubna, September 27, 2006 Relativistic.

Hadrons: color singlets “white states”

Light nuclei production in heavy-ion collisions at RHIC Md. Rihan Haque, for the STAR Collaboration Abstract Light nuclei (anti-nuclei) can be produced.

Study of Electromagnetic Interactions of Light Ions in the Framework of the IHEP Ion Program at U70 Serguei Sadovsky, IHEP, Protvino EMIN-2009, Moscow,

Modeling of the set-up for the Project experimental tasks and study of radiation hazard due to lost beam particles in the GSI Future Facilities INTAS-3588.

Atomic Number Proton Electron ELEMENTAtomic #Atomic MassProtonsNeutronsElectrons N K Ag Na O Ne Al

Atomic Structure Test Review 166 point total. 1.The atomic number is the number of protons. 2. The mass number is the number of protons and neutrons.

H.Sakurai Univ. of Tokyo Spectroscopy on light exotic nuclei.

High-resolution experiments on nuclear fragmentation at the FRS at GSI M. Valentina Ricciardi GSI Darmstadt, Germany.

Implantation of heavy ions 86 Kr and 132 Xe in emulsion with energy 1.2 A MeV K.Z. MAMATKULOV LHEP, JINR, Dubna, Russia. DjPI, Uzbekistan. “Workshop on.

Light nucleus clustering in fragmentation above 1 A GeV N. P. Andreeva a, D. A. Artemenkov b,V. Bradnova b, M. M. Chernyavsky c, A. Sh. Gaitinov a, S.

EURISOL – Task 11 meeting 2007S. Chabod 1 OUR CONTRIBUTION INSIDE EURISOL TASK 11 OPTIMIZATION OF IN-TARGET NUCLEI YIELDS Target parameters: material (Al.

Mitja Majerle for the “Energy Plus Transmutation” collaboration.

13-jan-2014 Some results for a GEM-based central detector A.Zinchenko, V.Vasendina, M.Kapishin VBLHEP, JINR, Dubna, Russia.

01/anthropology.jpg.

1 Study of 7 Be relativistic fragmentation in nuclear track emulsion Denis Artemenkov, VBLHE, JINR ( for the BECQUEREL collaboration )

Signals of bimodality in fragmentation induced by 3.65 A GeV 12C B.Grabez Institute of Physics Zemun.

NUCLEAR FRAGMENT SEARCH IN HADRON INTERACTIONS JIRO KAWADA(LHEP, BERN) ANIS BEN DHAHBI (F.S.T *, LHEP) JONAS KNUESEL (LHEP) * Faculty Science of Tunis.

What are the names of these elements? C O Na Li Fe Mg Pb Ca F Xe Ti K Ba B Si P Cl Be.

The BECQUEREL Project: Progress Report for Years and Plans for D. A. Artemenkov, V. Bradnov, A. I. Malakhov, D. O. Krivenkov, P. A. Rukoyatkin,

Momentum distributions of projectile residues: a new tool to investigate fundamental properties of nuclear matter M.V. Ricciardi, L. Audouin, J. Benlliure,

Itzhak Tserruya Initial Conditions at RHIC: an Experimental Perspective RHIC-INT Workshop LBNL, May31 – June 2, 2001 Itzhak Tserruya Weizmann.

OPERA Experiment, Brick Finding Program A. Chukanov Joint Institute for Nuclear Research Dubna, 25 th January, 2007.

FRAGMENTATION OF RELATIVISTIC 10 C NUCLEI IN NUCLEI EMULSION K. MAMATKULOV JINR, Dubna September.

A.Kubarovsky, V.Popov Observation of narrow exotic baryon resonance by the SVD-2 experiment in pA interactions at 70 GeV/c HSQCD 21 May 2004 Observation.

IMPLANTATION OF 8 Нe NUCLEI IN NUCLEAR TRACK EMULSION K.Z. MAMATKULOV LHEP, JINR, Dubna, Russia. DjPI, Uzbekistan. “Workshop on Nuclear Track Emulsion.

Fragmentation of relativistic 9 Be and 14 N nuclei in nuclear track emulsion D. A. Artemenkov JINR, Dubna BECQUREL Collaboration web site:

New results from Delia Hasch DPG Spring Meeting 2004 – Nuclear Physics Cologne (Germany) March, (on behalf of the HERMES Collaboration) Exotic.

Atomic notation X A Z X = Symbol (C, Au) A = Atomic Mass Number = #nucleons (Protons + Neutrons) Z = Atomic Number = #protons C 12 6 Carbon A = 12, Z =

SP- 41 magnet ZDC RPC (TOF) DC ST Target T0 detector MPD / NICA and / Nuclotron Experiments Picosecond Cherenkov detectors for heavy ion experiments.

Systematic Investigation of the Isotopic Distributions Measured in the Fragmentation of 124 Xe and 136 Xe Projectiles Daniela Henzlova GSI-Darmstadt, Germany.

Исследование кластеризации легких ядер в релятивистской фрагментации П.И. Зарубин (ОИЯИ, Дубна) N. P. Andreeva a, D. A. Artemenkov b,V. Bradnova b, M.

Investigation of Coherent Dissociation 10 C Nuclei at an Energy of 1.2 A GeV Mamatkulov Kahramon LHEP, JINR, Dubna JSPI, Uzbekistan EMIN’ October.

Gruppo di Napoli A. Aleksandrov, G. De Lellis, A. Di Crescenzo, M. Fioranelli, A. Iacomino, A. Lauria, J. Lotti, M.C. Montesi, V. Tioukov 1. Detector structure.

Electronegativity What is it? Electronegativity is the power of an atom to attract electron density Remember the definition … … look for where you get.

for the LNL-Ganil collaboration

Experimental data: Method:

L. Acosta1, M. A. G. Álvarez2, M. V. Andrés2, C. Angulo3, M. J. G

“It is better to begin in the evening than not at all”

August 31 – September 4, 2015, Groningen, Netherlands

Статус проекта БЕККЕРЕЛЬ и планы

of secondary light ion beams

of secondary light ion beams

Global Beam Energy Scan Global Beam Energy Scan

Search for unbound excited states of proton rich nuclei

A B 21085At Fe Mo 5827Co 3216S Pb4+ Symbol

GSI-Darmstadt, Germany

Michael Hass - Star Dust-אבק כוכבים

Fragmentation cross sections of Fe26+, Si14+ and C6+ ions of 0

Sakashita, Kouichi Shibata Laboratory

Topology rapidity study

Daniela Henzlova GSI-Darmstadt, Germany

Presentation transcript:

Topology of “ white ” stars in relativistic fragmentation of light nuclei in nuclear track emulsion P. I. Zarubin (JINR, Dubna)

0.5 μm resolution, identification of charges and H&He isotopes Au plate

3.65A GeV 28Si in emulsion AVI MOV

3.65A GeV 28Si 2+2+2+2+2+2+1

3.65A GeV 24Mg 2+2+2+2+2+2

bik=-(Pi/mi-Pk/mk)2

4.5A GeV/c 24Mg 5+2+2+1+1+1

4.5A GeV/c 24Mg 7+2+1+1+1

3.65A GeV 24Mg

3.3A GeV 22Ne 1400 inelastic stars

3.65A GeV 28Si

3.65A GeV 32S

3.65A GeV 28Si 1980 Inelastic Events

Q’=(M*-M)/A

3.65A GeV 20Ne 2+2+2+2+2

Tα 0.05-2 МэВ βα 0.005-0.03 Pα 20-110 MeV λ 10-2 fm

4.5 A GeV/c 16O

4.5A GeV/c 16O

2.1 А ГэВ 14N→3He+H jpg

3.65A GeV/c 14N

1A GeV 56Fe

158 A ГэВ/c Pb

158 A ГэВ/c Pb

158 A ГэВ/c Pb 1 2 AVI MOV 3 4

158 A ГэВ/c Pb 1 2 3 4 5 6

158 A ГэВ/c Pb 1 2 3 4

Au 10.6 A ГэВ 2 1 4 3

http://becquerel.jinr.ru/