DocumentCode
1403681
Title
Impact of the Residual Resistivity Ratio on the Stability of
Magnets
Author
Bordini, B. ; Bottura, L. ; Oberli, L. ; Rossi, L. ; Takala, E.
Author_Institution
Technol. Dept., CERN, Geneva, Switzerland
Volume
22
Issue
3
fYear
2012
fDate
6/1/2012 12:00:00 AM
Firstpage
4705804
Lastpage
4705804
Abstract
The CERN Large Hadron Collider (LHC) is envisioned to be upgraded in 2020 to increase the luminosity of the machine. The major upgrade will consist in replacing the NbTi quadrupole magnets of the interaction regions with larger aperture magnets. The Nb3Sn technology is the preferred option for this upgrade. The critical current density Jc of Nb3Sn strands have reached sufficiently high values (in excess of 3000 at 12 T and 4.2 K) allowing larger aperture/stronger field magnets. Nevertheless, such large Jc values may cause magneto-thermal instabilities that can drastically reduce the conductor performance by quenching the superconductor prematurely. In Nb3Sn magnets, a relevant parameter for preventing premature quenches induced by magneto-thermal instabilities is the Residual Resistivity Ratio (RRR) of the conductor stabilizing copper. An experimental and theoretical study was carried out to investigate how much the value of the RRR affects the magnet stability and to identify the proper conductor specifications. In this paper the main results are presented and discussed.
Keywords
niobium alloys; superconducting magnets; superconducting materials; tin alloys; CERN Large Hadron Collider; Nb3Sn; aperture magnet; conductor specification; conductor stabilizing copper; machine luminosity; magnet stability; magnetic flux density 12 T; magneto-thermal instabilities; quadrupole magnet; residual resistivity ratio; superconductor quenching; Conductors; Copper; Critical current; Current measurement; Magnetic field measurement; Niobium-tin; Superconducting magnets; ${rm Nb}_{3}{rm Sn}$ ; Magnet; RRR; stability;
fLanguage
English
Journal_Title
Applied Superconductivity, IEEE Transactions on
Publisher
ieee
ISSN
1051-8223
Type
jour
DOI
10.1109/TASC.2011.2180693
Filename
6109328
Link To Document