Storage ring at HIE-ISOLDE Technical design report
read more
Citations
Advanced multiconfiguration methods for complex atoms : I. Energies and wave functions
Facilities and methods for radioactive ion beam production
Nuclear fission: a review of experimental advances and phenomenology.
Physics book: CRYRING@ESR
Review of metastable states in heavy nuclei
References
Frequency Ratio of Al+ and Hg+ Single-Ion Optical Clocks; Metrology at the 17th Decimal Place
Microchannel plate detectors
The Nubase evaluation of nuclear and decay properties
Table of Nuclear Magnetic Dipole and Electric Quadrupole Moments
Related Papers (5)
The GSI projectile fragment separator (FRS): A Versatile magnetic system for relativistic heavy ions
Frequently Asked Questions (22)
Q2. What are the ideal probes for the measurement of nuclear properties?
In particular, Li-like ions and with some restrictions Na-like ions provide ideal probes for the measurement of nuclear properties such as charge radii, magnetic moments and nuclear spins.
Q3. What is the key uncertainty in determining the astrophysical reaction rate?
For resonances in such reactions the proton spectroscopic factor is often the key uncertainty in determining the astrophysical reaction rate.
Q4. Why is a superior energy resolution expected in reaction measurements with an internal target?
Because of the very good beam-energy definition and the absence of straggling in the target, a superior energy resolution is expected in reaction measurements with an internal target: the remaining contributions would be the intrinsic resolution of the charged-particle detectors and the spatial resolution affecting the kinematical reconstruction; for the latter, good collimation of the beam on the target is necessary.
Q5. How much air is needed to prevent the magnet poleshoes from overheating?
A pressure of 2 bar and a continuous stream of about 20m3/h of air is considered to be sufficient to prevent the magnet poleshoes from overheating.
Q6. How many tungsten ions can be supplied in sufficient quantities for DR experiments?
With the present configuration of MPIK accelerators, tungsten ions with charge states of about up to 30+ can be supplied in sufficient quantities for DR experiments.
Q7. How fast can a ramping speed be made?
Ramping can be made to accelerate or decelerate the stored ion beams, however, with present power supplies only a relatively slow ramping speed is possible (a few seconds from Min to Max).
Q8. How can the schottky signal be used to determine the tune of the storage?
The transverse Schottky signal can be used todetect transversal coherent oscillations of the stored ion beam at high intensities, as well as the tune of the storage ring can be determined by analyzing the position of the two sidebands in the transversal Schottky spectrum.
Q9. How can the charge state of the ions be increased?
By introducing a carbon stripper foil (thickness of ∼150µg/cm2) at the end of the linac the charge state of the ions can be increased in certain cases.
Q10. What is the time required to reach a certain charge state?
In other words, the time required to reach a certain charge state depends on the electron-impact ionization cross-sections and the electron beam current density.
Q11. How long after injection does the noise transfer to the horizontal kicker take place?
– Between 1.3 s and 1.8 s after injection: After 1.3 s noise is transferred to the horizontal kicker blowing up the transverse phase of the stored ion beam, recognizable in the increase of the beam size.
Q12. What is the cooling time for a multiturn injected proton beam?
This means the cooling time for a multiturn injected proton beam in the velocity range between 0.03 < β < 0.16 is about 3 s.The equilibrium emittance and momentum spread of an electron cooled ion beam is determined by the electron cooling force and the intra-beam scattering, which is heating the stored ion beam.
Q13. What is the lifetime of the ions due to the electron capture in the gas?
According to Eq. (28) the lifetime due to the electron capture in the residual gas is much stronger energy dependent than the lifetime of single- and multiple-scattering processes.
Q14. What is the reason why the decays of ionized atoms are disabled?
It is obvious, that the electron capture and electron conversion decays are disabled in the absence of orbital electrons in fully-ionized atoms.
Q15. What was the maximum voltage of the rf-stacked ion beam?
The design criteria of the maximum voltage of 5 kV was the demand of adiabatic capture of an rf-stacked ion beam having a momentum spread of about 1%.
Q16. How many kAs/cm2 is required to reach these high charge states?
Simulations using CBSIM [214], shown in Fig. 19, indicate that a je · T in excess of 20 kA·s/cm2 is required in order to reach these high charge states.
Q17. How long does the ion throughput in REXTRAP take to be reduced?
If a long storage time in REXTRAP (forinstance 1.5 s) is requested due to the electron cooling time in TSR, the ion throughput will be correspondingly lower (∼3 · 106 ions/s).
Q18. How small is the space between the ferrite rings and the quadrupole poles?
In order to reduce the necessary d.c. power the space between the ferrite rings and the quadrupole poles must be as small as possible.
Q19. How can the storage lifetimes of 7Be3+ be accurately calibrated?
The storage lifetimes as well as the cross-sections for electron pick-up and stripping can be accurately calibrated with stable Li and Be ions in all required charge states.
Q20. What is the way to measure isomeric lifetimes?
The latter option is very attractive since isomeric lifetimes can be measured in dependence on a well-controlled degree of ionization, i.e., with partial or full suppression of internal conversion or nuclear electron capture.
Q21. How does TSR solve the problem of storing ions long enough for EII studies?
TSR overcomes this issue by storing the ions long enough for metastable levels to radiatively relax, thereby generating a ground state beam of ions for EII studies and unambiguous benchmarking of theory.
Q22. What is the density of s-electrons in L, M and higher atomic?
In a simple picture the density of s-electrons in L, M and higher atomic shells scales as 1/n3 (n is the principal quantum number).