Umlauffrequenz der Ionen im ESR liegt bei 2 . 106 s-1. Der Druck im Inneren des Systems liegt bei 10-11 mbar, damit möglichst wenig Kollisionen zwischen Ionen und Restgasmolekülen auftreten. Um den Strahl [...] GHz installed CW power 2.4 kW longitutinal cooling: Palmer, TOF or notch filter vacuum Operational 10-11 mbar bakeable up to 300 °C beam diagnostics 12 position monitors dc transformer fast current transformer

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t for heavy atom nanoparticles irradiated by protons, Phys. Med. Biol., 59:1441-1458 (2014); DOI: 10.1088/0031-9155/59/6/1441 [2] Tinganelli W., Durante M., Hirayama R., Krämer M., Maier A., Kraft-Weyrather [...] stage extension of the particle track structure code TRAX in water targets. Chem. Phys. Lett. 698, 11-18 (2018) [7] Sokol O., Krämer M., Hild S., Durante M., Scifoni E., Kill painting of hypoxic tumors

innovation, 4.12.2023 Startup-Afternoon, 30.11.2023 HEPTrepreneurs Training School @GSI/FAIR, 29.11.2023 GSI and FAIR at Start-up & Innovation Day 2023 , 02.11.2023 Open Data Center Day , 26.10.2023 Where [...] 2023 Roadshow 15.12.2022 Roadshow 24.11.2022 Transfer NEWS: "Datacenter Strategy Award", 09.11.2022 "HEPTrepreneurs Episode 10 - How to write a Business Plan", 09.11.2022 GSI/FAIR news about the Darmstadt [...] mance computing center Green IT Cube — DC Smarter and GSI/FAIR cooperate Roadshow 11.05.2023 HEPTrepreneurs Episode 11 - Cold Atmospheric Plasma: from lab to the clinic, 04.04.2023 European Cryogenic Days

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Kontrolle des dynamischen Vakuums im SIS100 ( German ) Dissertation L. Bozyk, June 2012, TU Darmstadt, 151 Pages; If you have any further questions or remarks, please send an email to Webmaster@SIS100

University in Frankfurt. Our address is: Giersch Science Centre Max-von-Laue-Straße 12, Offices: 3/10 and 3/11 60438 Frankfurt am Main, Germany How to get to us by public transport? The Uni Campus Riedberg stop

Central wavelength 1030 nm 515 nm Pulse duration (FWHM) 3.5 ps, 275 ps or 0.4 ns – 10 ns ≈ Original/1.41 Signal to PHELIX emission ratio Not measured > 110 Temporal pulse shape Gaussian like < 0.4 ns & >

Space-Charge Driven Emittance Growth in a 3D Mismatched Anisotropic Beam . Physical Review Letters 92, 174801 (2004) P. Zenkevich, A. Dolinsky, I. Hofmann: Dipole instability of a circulating beam due to the [...] driven resonance trapping observed at the CERN proton synchrotron . Phys. Rev. ST Accel. Beams 6, 124201 (2003) E. Mustafin, I. Hofmann, H. Weick: Influence of electronic stopping power on the total neutron

Instr. Meth. A 593, 171-176 (2008) O. Boine-Frankenheim, V. Kornilov, S. Paret: Measurement and simulation of the transverse Schottky noise with space charge . Phys. Rev. ST Accel. Beams 11, 074202 (2008) A [...] Transverse Schottky noise spectrum for bunches with space charge . Phys. Rev. ST Accel. Beams 12, 114201 (2009) M. Eshraqi, G. Franchetti, A. Lombardi: Emittance control in RF cavities and solenoids . Phys [...] Zimmermann: Incoherent effect of space charge and electron cloud . Phys. Rev. ST Accel. Beams 12, 124401 (2009) I. Strasik, E. Kozlova, E. Mustafin, I. Hofmann, A. Smolyakov, N. Sobolevskiy, L. Latysheva