The HiLumi LHC Design Study is included in the High Luminosity LHC project and is partly funded by the European Commission within the Framework Programme.

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Presentation transcript:

The HiLumi LHC Design Study is included in the High Luminosity LHC project and is partly funded by the European Commission within the Framework Programme 7 Capacities Specific Programme, Grant Agreement WP6.4 – Updates on Dose and Dpa studies on SC Links at P1 Carlo Santini (Politecnico di Milano, INFN) 4 nd Joint HiLumi LHC-LARP Annual Meeting Tsukuba November 2014

Tsukuba November 20th Outlines SC Link in P1 layout SC Link in P1 layout SC Link: real structure and simulated layout SC Link: real structure and simulated layout Critical points Critical points First quadrupole region: results and analysis First quadrupole region: results and analysis Shuffling Module region: results and analysis Shuffling Module region: results and analysis Conclusions Conclusions

P1 3Tsukuba November 20th 2014 Possible disposition of the SC link in the FLUKA simulation of P1 geometry The link will start its run from the surface and will enter in ATLAS cave between the interaction point and the Q1. Than it will run parallel to the beam line at about one meter from the quadrupoles. At the end it will enter in the shuffling module (located at about 80 m from the IP1).

Tsukuba November 20th SC Link Structure Sub-unit of 18 MgB 2 (green) wires around a Cu (red) bulk Φ = 6.5 mm 20 kA cable 6 sub-unit around a steel (grey) tube Φ = 19.5 mm Concentric 2×3 kA cable (Kapton in orange) Φ = 8.4 mm 0.4 kA cable Φ = 3 mm 0.12 kA cable Φ = 3 mm 165 kA cable assembly (6×20 kA, 7×2×3 kA, 4×0.4 kA, 18×0.12 kA) Φ = 65 mm (white regions are flled with 20 K Helium) Amalia Ballarino

Tsukuba November 20th SC Link in FLUKA Real Link simulated in FLUKA. We used this configuration for the P1 simulations. Real SC Link Simulated SC Link

Tsukuba November 20th Critical Points First Quadrupole: this is the quadrupole closest to the interaction point and here there will be the highest debris. First Quadrupole: this is the quadrupole closest to the interaction point and here there will be the highest debris. Shuffling Module: in this region the SC link will pass very close (about 20 cm) to the beam pipe. Shuffling Module: in this region the SC link will pass very close (about 20 cm) to the beam pipe.

Tsukuba November 20th First Quadrupole Region The SC Link will run parallel to the first quadrupole at about 1 m distance.

Daresbury November 13th Particles Entering SC Link (10 m) Q1 7.6∙10 18 particles/3000 fb -1 High number of neutrons

Tsukuba November 20th Q1 Dose & Dpa Peaked dose trends: the link is 10 meters long so there will not be an uniform deposition along the length of the cable Dpa trends are more regular thank to the high number of neutrons impinging on the link

Tsukuba November 20th Q1 Neutron Fluence Very similar trends Neutron FluenceDpa

Tsukuba November 20th Q1 Analysis The region presents a not optimal statistic due to the low number of particles impinging. The particles are not uniformly distributed along the length of the link ( except for neutrons which are enough to produce a good fluence trend and so a good dpa trend). The region presents a not optimal statistic due to the low number of particles impinging. The particles are not uniformly distributed along the length of the link ( except for neutrons which are enough to produce a good fluence trend and so a good dpa trend). The maximum dose and maximum dpa values are low and the statistical error is under 20%. The maximum dose and maximum dpa values are low and the statistical error is under 20%.

Tsukuba November 20th Shuffling Module Region The SC link will enter in the shuffling module from above (vertical cable) and than will lay on the bottom (horizontal cable) before been separated in his components and connected to the loads.

Tsukuba November 20th Particles Entering SC Links (2x1m) SM 3.4∙10 19 particles/3000 fb -1 High number of photons

Tsukuba November 20th SM Vertical Cable Dose & Dpa Good trends: the high number of particles impinging on the same bins gives an excellent statistic Peaks due to the dpa in air: they must be ignored ERR 50%

Tsukuba November 20th SM Vertical Cable Fluences

Tsukuba November 20th SM Vertical Cable Fluences

Tsukuba November 20th SM Horizontal Cable Dose & Dpa The circled peaks are due to very energetic Single Events which don’t permit a good statistical convergence of the results: they can be neglected ERR 30% ERR 41% ERR 27%

Tsukuba November 20th SM Horizontal Cable Fluences The number of neutrons and photons impinging on the SC Link are enough to generate good trends along the length of the cable

Tsukuba November 20th SM Horizontal Cable Fluences The little number of pions and protons impinging on the SC Link causes irregular trends

Tsukuba November 20th SM Analysis In the vertical cable the trends are regular and the errors are very low. In the vertical cable the trends are regular and the errors are very low. In the horizontal cable there are some Single Events that cause anomalous peaks with high error (greater than 20%) that can be neglected for an integrated analysis. In the horizontal cable there are some Single Events that cause anomalous peaks with high error (greater than 20%) that can be neglected for an integrated analysis. Being the maximum dose and maximum dpa in the vertical section of the SC link we will focus on the vertical cable for the Shuffling Module region. Being the maximum dose and maximum dpa in the vertical section of the SC link we will focus on the vertical cable for the Shuffling Module region.

Tsukuba November 20th Conclusions RegionMax Dpa [dpa]Err%Max Dose [MGy]Err% First Quadrupole1.97∙ Shuffling Module3.11∙ The maximum values in both the critical regions are very low: ● the dose shows a peak of 3.3 MGy when the design limit for the SC Link (precisely for the kapton) is 50 MGy ● the dpa maximum is of the order of magnitude of that will be probably under the safety threshold (not yet defined) The SC links in the P1 will live until the dead of HL-LHC

Tsukuba November 20th Acknowledgment 感謝 A. Ballarino F. Cerutti, L. S. Esposito