Lasers and Highly-Charged Heavy Ions

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Lasers and Highly-Charged Heavy Ions at Günther Rosner HZDR Workshop, Rossendorf, 6/9/11 1

description

Lasers and Highly-Charged Heavy Ions. at. F acility for A ntiproton and I on R esearch. FAIR. Nuclear Structure & Astrophysics (Rare-isotope beams). Hadron Physics (Stored and cooled 14 GeV/c anti-protons). SIS18. p-Linac. SIS100 /300. UNILAC. QCD-Phase Diagram - PowerPoint PPT Presentation

Transcript of Lasers and Highly-Charged Heavy Ions

Page 1: Lasers  and Highly-Charged  Heavy  Ions

Lasers andHighly-Charged Heavy Ions

at

Günther Rosner HZDR Workshop, Rossendorf, 6/9/11 1

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Facility for Antiproton and Ion Research

Günther Rosner HZDR Workshop, Rossendorf, 6/9/11 2

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FAIR

Günther Rosner HZDR Workshop, Rossendorf, 6/9/11

Dense Bulk Plasmas (Ion-beam bunch compression& petawatt-laser)

Materials Science & Radiation Biology (Ion & antiproton beams) Accelerator Physics

UNILAC

SIS18 SIS100/300p-Linac

HESR

CR &RESR

NESR

Cryring

Rare-IsotopeProduction Target

Anti-ProtonProduction Target

100 m

QCD-Phase Diagram(HI beams 2 to 45 GeV/u)

Hadron Physics (Stored and cooled14 GeV/c anti-protons)

Nuclear Structure & Astrophysics(Rare-isotope beams)

Fundamental Symmetries& Ultra-High EM Fields(Antiprotons & highly stripped ions)

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HZDR Workshop, Rossendorf, 6/9/11 4

Parallel Operation

Günther Rosner

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Experiments

Günther Rosner HZDR Workshop, Rossendorf, 6/9/11

CBM

PANDA NuSTAR

Super-FRS

APPA

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PANDA

Günther Rosner HZDR Workshop, Rossendorf, 6/9/11

PANDA

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Compressed Baryonic Matter

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SIS100/300

ALICE @ CERN

CBM @ FAIR

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NuSTAR

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APPA• Atomic Physics, Fundamental Interactions,

High EM Field Physics (SPARC)– Weak interactions in parity-violating atomic transitions– High field QED in bound system– Pair production

• Plasma Physics, Planetary Astrophysics– Warm Dense Matter (WDM) &

High Energy Density Matter (HEDgeHOB)– Plasma astrophysics in the lab

• Nuclear Physics– Measurement of nuclear moments – Nuclear excitation by laser excitation (NEET)

• Applied Physics, Accelerator Science– Integrated concept for laser-acceleration applications

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HZDR Workshop, Rossendorf, 6/9/11 10

Staging

Günther Rosner

Start Version Phase A(SIS100) Phase B

(SIS300)

Modularised Start Version

Module 0 Module 1 Module 2 Module 3 Module 4 Module 5

SIS100 Exp. halls for CBM &

APPA

Super-FRS for

NuSTAR

Antiproton Facilityfor PANDA & options for

NuSTAR

LEB, NESR, FLAIR

for NuSTAR & APPA

RESRfor PANDA, NuSTAR &

APPA

2017/18

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HZDR Workshop, Rossendorf, 6/9/11 11

Modularised Start Version

Günther Rosner

APPA

CBM/HADES

NuSTAR

PANDA

ExperimentsM1: APPAM1: CBM/HADESM2: NuSTARM3: PANDA

M0

M1

M2M3

M3

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HZDR Workshop, Rossendorf, 6/9/11 12

Timelines

Günther Rosner

20122011 2013 201620152014

6

Building permitsSite preparationCivil construction contractsBuilding of accelerator & detector componentsCompletion of civil construction workInstallation of accelerators and detectorsData taking

7 108

2017 2018 2019

12

6

789

11

12

10

119

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Lasers & HI Accelerators

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Advanced particle accelerators

(e.g. @ GSI and FAIR)

"... thus the technologies are complementary [intense light sources and ion beams] and both are likely to lead to new insights in high-intensity science."

National Research Council, USA, 2008

Novel lasers: Vulcan, POLARIS, DRACO,

PHELIX, ELI

Free electron lasers (e.g. LCLS @ SLAC)

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Parity-Violating Transitions in Atoms

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PS

PNWFS

EE

QG

522/

Mixing coefficient for states with opposite parities:

Energy levels of He-like uranium

2E1 (PNC)

To “compete” with spontaneous decay channels one needs to

induce a two-photon PNC transition by polarised light with

intensity 1020 W/cm2

NN

ee

Zee

NN

Select case with small splitting!

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Extreme EM Fields

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Sub-femtosecond pulses

Heavy ions

Large EM fields,zeptosecond pulses

Equivalent toI ≥ 1028 W/cm2

Lasers

(adapted from Mourou, Tajima, Bulanov, RMP 78, 2006)

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Relativistic HI EM Fields

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The electric field produced by a moving charge (>>1) is nearly transverse (linearly polarised) and is accompanied by a transverse magnetic field of almost equal strength.

Parameters of the “pulse”:

@ FAIR:

vbt /

bc /

MeVzsst

800110 21

E

BU92+

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Plasmas

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Particles / cm-3

Tem

pera

ture

[eV

]

Jupiter

LaserHeating

Sun Surface

Magnetic Fusion

solid statedensity

PHELIXSun Core

Inertial Fusion Energy

XFEL

SIS 18

Ion BeamHeating

SIS 100

Strongly coupled

plasmasIdeal plasmas

FLASH

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Heavy-Ion beams at FAIR and novel XUV photon sourcesprovide complementary tools:

Specific energy ~ kJ/g

Temperature up to 1 eV

Pressure multi-kbar

range

High-brilliance XUV photon sources (FLASH@DESY)

small sample volume (100 m3) high gradients

low-Z target materialshort time scales (100 fs)

Intense, energetic beams of heavy ions (GSI & FAIR)

large sample volume (mm3)uniform physical conditions

any target materiallong time scales (50 ns)

65 mmNe10+ 300 MeV/u; Kr crystal

WDM & HEDgeHOB @ FAIR

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Laser beam

Laser-accelerated protons

Laser-generated X-ray or proton diagnostics @ FAIR

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Laser beam

X-rays coherent (XRL)or incoherent

back-lighter target

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2P3/2

2S1/2

2P1/2

...allows for precision tests of QED, atomic physics and nuclear models...

50 60 70 80 900

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

Nuclear Charge Z

13,9nm/89eV (Ag)

14,7nm/84eV (Pd)

18,9nm/66eV (Mo)

22,0nm/56eV (Zr)

Steerer-Magnets (7,2 Tm)

Electron Cooler (240 kV)

ESR-Magnets (10 Tm)

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Spectroscopy of Lithium-like Ions

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Larger Doppler-Boost @ HESR, =5

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Back-scattered laser radiation from a compact electron ring (e.g. semi-commercial „Lyncean Compact Light Source“ would reach well above 100 keV.

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Laser-Accelerated Protons & Conventional AcceleratorsJoint research project@ GSI • Helmholtz Institute Jena:

Project coordination, 100TW compressor, short laser pulse and ion beam diagnostics

• GSI: PHELIX Laser, timing, control system, beamlines, accelerator structures, beam diagnostics

• FZ Dresden-Rossendorf: Solenoid for collimation & PSU

• TU Darmstadt: Acceleration experiments, collimation simulations, target development

• Univ. Frankfurt: Accelerator structure development

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Thank you very much!

Günther Rosner HZDR Workshop, Rossendorf, 6/9/11 23