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"Tomography" of nuclear "Tomography" of nuclear structure in dissociation of structure in dissociation of relativistic nuclei relativistic nuclei P. I. Zarubin P. I. Zarubin V. I. Veksler and A. M. Baldin Laboratory of High Energy Physics V. I. Veksler and A. M. Baldin Laboratory of High Energy Physics Joint Institute for Nuclear Research, Dubna, Russia Joint Institute for Nuclear Research, Dubna, Russia The use of accelerated nuclei, including radioactive ones, qualitatively diversifies the spectroscopy of cluster systems. Configuration overlap of a fragmenting nucleus and finite cluster states manifests in the dissociation at the periphery of the target nucleus. The definition of interactions as peripheral ones is simplified at energy above 1A GeV due to the collimation of the incident nucleus fragments. The detection
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"Tomography" of nuclear structure in dissociation of relativistic nuclei P. I. Zarubin

Jan 03, 2016

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"Tomography" of nuclear structure in dissociation of relativistic nuclei P. I. Zarubin V. I. Veksler and A. M. Baldin Laboratory of High Energy Physics Joint Institute for Nuclear Research, Dubna, Russia - PowerPoint PPT Presentation
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Page 1: "Tomography" of nuclear structure in dissociation of relativistic nuclei  P. I. Zarubin

"Tomography" of nuclear structure "Tomography" of nuclear structure in dissociation of relativistic nuclei in dissociation of relativistic nuclei

P. I. Zarubin P. I. Zarubin V. I. Veksler and A. M. Baldin Laboratory of High Energy PhysicsV. I. Veksler and A. M. Baldin Laboratory of High Energy Physics

Joint Institute for Nuclear Research, Dubna, RussiaJoint Institute for Nuclear Research, Dubna, Russia

The use of accelerated nuclei, including radioactive ones, qualitatively diversifies the spectroscopy of cluster systems. Configuration overlap of a fragmenting nucleus and finite cluster states manifests in the dissociation at the periphery of the target nucleus. The definition of interactions as peripheral ones is simplified at energy above 1A GeV due to the collimation of the incident nucleus fragments. The detection thresholds disappear and energy lose in detector material are minimal.

Page 2: "Tomography" of nuclear structure in dissociation of relativistic nuclei  P. I. Zarubin
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2424Mg Mg → 6→ 6αα

2222Ne → 5Ne → 5αα

1616O → 4O → 4αα

1212C → 3C → 3αα

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The use of accelerated nuclei, including radioactive ones, The use of accelerated nuclei, including radioactive ones, qualitatively diversifies the cluster spectroscopy. Configuration qualitatively diversifies the cluster spectroscopy. Configuration overlap of a fragmenting nucleus and final cluster states overlap of a fragmenting nucleus and final cluster states manifests in the dissociation at the periphery of the target manifests in the dissociation at the periphery of the target nucleus. The definition of interactions as peripheral ones is nucleus. The definition of interactions as peripheral ones is simplified at energy above 1A GeV due to the collimation of the simplified at energy above 1A GeV due to the collimation of the fragments. The detection thresholds disappear and energy lose fragments. The detection thresholds disappear and energy lose in detector material are minimal. in detector material are minimal. These statements are These statements are particularly true for the light nuclei with an excess of protons.particularly true for the light nuclei with an excess of protons.

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Internal target

Experimental hall 1B

Experimental hall 205

Experimental hall

NUCLOTRON – 6 GeV/n

SYNCHROPHASOTRON

CO2 laserCO2 laser

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2A GeV/2A GeV/cc 99Be Be → 2→ 2αα “white” star “white” star

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<<PPTT**>=52 >=52 MeV/cMeV/c

EMD “white”starsEMD “white”stars

nnhh≠≠00

88B B → → 77Be + pBe + p

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33He (He (hh) ) – – helion helion 2233He (He (22hh) ) –– dihelion dihelion?!...?!...

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160A GeV Pb160A GeV Pb

10A10A GeV Au GeV Au

1A1A GeV U GeV U

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1.2A GeV 9Be 3.22A GeV 22Ne 10.7A GeV 197Au

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Request for irradiation to a high-energy muon beam

• Until now, a high-energy muon exposure has not been conducted, which is a Until now, a high-energy muon exposure has not been conducted, which is a notable omission in survey observations of high-energy particle interactions. notable omission in survey observations of high-energy particle interactions.

• Meanwhile, the use of the muon, which is an electromagnetic probe, facilitates Meanwhile, the use of the muon, which is an electromagnetic probe, facilitates the interpretation of the phenomenon of nuclear multiple fragmentation.the interpretation of the phenomenon of nuclear multiple fragmentation.

• Moreover, the unexplored effects of multiphoton exchange may occur in the Moreover, the unexplored effects of multiphoton exchange may occur in the formation of muon stars associated with the destruction of heavy nuclei of formation of muon stars associated with the destruction of heavy nuclei of emulsion. emulsion.

• In addition to the nuclear dynamics, the muon interactions associated with the In addition to the nuclear dynamics, the muon interactions associated with the electron-positron pair formation in strong electromagnetic fields of heavy electron-positron pair formation in strong electromagnetic fields of heavy nuclei can be studied. nuclei can be studied.

• It is also important that the images of the investigated events will complement It is also important that the images of the investigated events will complement the nuclear photo collection begun in the classic book by Powell, Fowler and the nuclear photo collection begun in the classic book by Powell, Fowler and Perkins. Perkins.

• In terms of applications the received material will be very valuable for the In terms of applications the received material will be very valuable for the development of systems of automatic search for nuclear interactions, as well as development of systems of automatic search for nuclear interactions, as well as for university educationfor university education.

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Hammer tracks inHammer tracks in cosmic ray events:cosmic ray events:

88Be produced inBe produced in ββ-delayed decay of -delayed decay of stopped stopped 88B and B and 88Li Li

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ConclusionsConclusionsThe presented observations serve as an illustration of prospects of the The presented observations serve as an illustration of prospects of the Nuclotron for nuclear physics and astrophysics researchesNuclotron for nuclear physics and astrophysics researches. . The relativistic The relativistic energy scale does not impede investigations of nuclear interactions down to energy scale does not impede investigations of nuclear interactions down to energy scale relevant for nuclear astrophysics, but on the contrary gives energy scale relevant for nuclear astrophysics, but on the contrary gives advantages for investigation of multi-particle systems. advantages for investigation of multi-particle systems.

Due to a record space resolution the emulsion technique provides Due to a record space resolution the emulsion technique provides unique entirety in studying of light nuclei, especially, neutron-deficient unique entirety in studying of light nuclei, especially, neutron-deficient ones. Providing the 3D observation of narrow dissociation vertices this ones. Providing the 3D observation of narrow dissociation vertices this classical technique gives novel possibilities of moving toward more and classical technique gives novel possibilities of moving toward more and more complicated nuclear systems. more complicated nuclear systems.

The results of the light nucleus study lead to the conclusion that The results of the light nucleus study lead to the conclusion that their structure dominates in very peripheral dissociations while some their structure dominates in very peripheral dissociations while some unknown features are clearly observed unknown features are clearly observed

The investigations with light nuclei provide a basis for challenging The investigations with light nuclei provide a basis for challenging studies of increasinglystudies of increasingly complicated systems complicated systems He – H - n He – H - n produced via produced via complete fragmentation of heaviest relativistic nuclei. complete fragmentation of heaviest relativistic nuclei.

Long and bright road is ahead for nuclear researches using HEP Long and bright road is ahead for nuclear researches using HEP techniques. Nuclear imaging continue to inspire our imagination.techniques. Nuclear imaging continue to inspire our imagination.

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““ССreative atmosphere of Lreative atmosphere of Lebedev ebedev Physical Instutute and my teachers have always Physical Instutute and my teachers have always given to understand: no quantitative results and formulas are the final products, but based on given to understand: no quantitative results and formulas are the final products, but based on them images and pictures of the processes.them images and pictures of the processes.””

А. М. А. М. BaldinBaldin ““Essay on a given topicEssay on a given topic”” (1996)(1996)““Творческая атмосфера ФИАН и мои учителя постоянно давали понять: не Творческая атмосфера ФИАН и мои учителя постоянно давали понять: не

количественные результаты и формулы являются конечными продуктами, а количественные результаты и формулы являются конечными продуктами, а созданные на их основе образы, картины процессов.созданные на их основе образы, картины процессов.””

А. М. Балдин А. М. Балдин ““Сочинение на заданную темуСочинение на заданную тему”” (1996 г.) (1996 г.)

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0.5 0.5 μμm resolutionm resolution, , identification of charges and H&He isotopesidentification of charges and H&He isotopes

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The unique collection of images in the “Emulsion Bible” by Powell,

Fowler, and Perkins.

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Interactions of relativistic nuclei of galactic originInteractions of relativistic nuclei of galactic origin

≈ ≈ 8A GeV Calcium8A GeV Calcium

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pβc for beam 3He nuclei, H fragments of the "white" stars ∑Zfr = 5 + 1 and4 + 1 + 1, He fragments of the "white" stars 3He and from the 33He event

δ -electrons density for beam particles and relativistic fragments with charges Zfr > 2 from "white" stars ∑Zfr = 5 + 1 and 4 + 1 + 1

Polar angles θ for doubly charged fragments in the "white" stars C 3He Opening angles Θ2Не between fragments in the "white" stars C 3He

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6Li 7.5% 7Li 92.5%

9Be 100%

10B 19.8% 11B 80.2%

12C 99%

7Be 53 d

8B 0.8 s

9C 0.13 s 10C 19 s 11C 20 m

12N 11 ms

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PT (7Li), GeV/c

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4.5 A GeV/c 16O

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4.5A GeV/c 641 events 4.5A GeV/c 641 events 1616O O → 4→ 4αα

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6He 807 ms 8He 119 ms

12Be 23 ms

12B 20 ms

10Be 1510000 y 11Be 13.8 s

8Li 838 ms

9Li 178 ms

11Li 8.5 ms0+ 0+

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Photo of human hair superposed on nuclear star inducedPhoto of human hair superposed on nuclear star induced by relativistic sulphur nuclei in nuclear track emulsionby relativistic sulphur nuclei in nuclear track emulsion

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Lebedev PI (FIAN)Lebedev PI (FIAN) 50-50-iesies….….

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22Ne 3.22A GeV4100 Inelastic Interactions

QQ’’=(M*-M)/A=(M*-M)/A

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10.7 A10.7 A GeV AuGeV Au

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