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What do we need? René Flükiger Dept. Phys. Cond. Matter (DPMC) & TE-MSC-SCD CERN WAMSDO 2011 Workshop (CERN), 14.11.111.

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Presentation on theme: "What do we need? René Flükiger Dept. Phys. Cond. Matter (DPMC) & TE-MSC-SCD CERN WAMSDO 2011 Workshop (CERN), 14.11.111."— Presentation transcript:

1 What do we need? René Flükiger Dept. Phys. Cond. Matter (DPMC) & TE-MSC-SCD CERN WAMSDO 2011 Workshop (CERN), 14.11.111

2 2 Starting point of the present considerations: Calculations of F. Cerutti (CERN), 2010 (newer calculations in his presentation, today) In the following, analysis will be restricted on Nb 3 Sn (quadrupoles) MgB 2 for current leads: talk of M. Putti BI-2212: not yet developed at an industrial level.

3 WAMSDO 2011 Workshop (CERN), 14.11.113 Neutron fluence in the inner winding of Quadrupoles (LHC Upgrade) « TRIPLET » Q1Q2aQ2bQ3 20 25 30 35 40 45 50 55 60 Distance from Collision Point (m) F. Cerutti + A.Mereghetti (CERN), 2010 Peak: > 5 x 10 17 neutrons/cm 2 Fluence in 10 « years » (200 days)

4 WAMSDO 2011 Workshop (CERN), 14.11.114 1 MeV Neutron spectrum in the inner coil of Q2a at peak location Neutrons

5 WAMSDO 2011 Workshop (CERN), 14.11.115 1 MeV 100MeV 1GeV Proton spectrum in the inner coil of Q2a at peak location Protons

6 WAMSDO 2011 Workshop (CERN), 14.11.116  1 GeV Pions + Pions - Pion spectrum in the inner coil of Q2a

7 WAMSDO 2011 Workshop (CERN), 14.11.117 Aperture 200mm 130mm130 mm Photons 88.93 89.00% Neutrons 4.82 4.04% 4.04% Protons 0.14 0.13%0.13% Pions+ 0.19 0.19% 0.19% Pions- 0.26 0.25% 0.25% Electrons 4.31 4.63% Positrons 2.23 2.45% Peak Fluence, LHC Upgrade (5 x 10 34 cm -2 s -1 ) Radiation spectrum at Q2a: 35m from Collision Point 0.57% Protons + Pions(+) + Pions(-) ≈ 14 % Neutrons

8 Question: How do the magnets (quadrupoles) behave after 10 years of operation? Study to be carried out for each high energy source: * the superconductorT c, J c, H c2 * the stabilizing Cu  (T) * the insulatormechanical properties, electrostatic charges,… * the magnetcombined effects, quench behavior, volume changes (expansion of Nb 3 Sn, Cu and insulator ) WAMSDO 2011 Workshop (CERN), 14.11.118

9 Keep in mind: * all high energy sources act simultaneously * there is no experience on a combined effect of several high energy sources * subsequent irradiations with different sources should be carried out on selected samples * calculations must be carried out to study combined irradiations (taking into account the small values of dpa, this may be possible WAMSDO 2011 Workshop (CERN), 14.11.119

10 10 Neutrons : Strong source of damage for superconductors Protons: From known data, even stronger effect (charge) Pions: Nothing is known yet. Effects expected to be comparable to those of protons (charges +/-) Electrons: Very little is known. Much smaller effects expected (in contrast to insulators). More data needed Photons: Nothing is known. Smaller effects expected. Data needed Known effects of radiation on superconductors

11 WAMSDO 2011 Workshop (CERN), 14.11.1111 What should be analyzed about irradiation of the superconductor? Damage Mechanism (atomic ordering); Comparison with heavy ion irradiation Effect of various energy sources Number of displacement per atoms Summation of single irradiations (small dpa numbers) Irradiation at 4.2K and 300K Volume expansion of Nb 3 Sn; Effect of repeated warming up and cycling on irradiated superconductors Thermal stabilization: Recovery behavior of Cu? Mechanical properties of the superconductor after irradiation

12 WAMSDO 2011 Workshop (CERN), 14.11.1112 Mechanisms of irradiation damage Due to limited data, results from heavy ion irradiation are also taken into account

13 High energy particle (n, p, p, heavy ions, fission fragments Frenkel defects, Vacancies, Interstitials Focused Collision Replacement Sequences Collision events (1 st, 2 nd, 3rd,…) Lattice expansionDisordering Antisite Defects Mean Static Displacements Depleted zones  a > 0  S > 0  ( ) 1/2 ≠ 0 Amorphous or transformed Increasing volume fraction Vacancy Clusters Vacancy mechanism Low Fluence High Fluence Building up of Internal strain (strain misfits) 13 R. Flükiger, 1986 WAMSDO 2011 Workshop (CERN), 14.11.11 13

14 WAMSDO 2011 Workshop (CERN), 14.11.1114 Effect of neutron irradiation on T c

15 WAMSDO 2011 Workshop (CERN), 14.11.1115

16 WAMSDO 2011 Workshop (CERN), 14.11.1116

17 A.R. Sweedler, D.G. Schweizer, G.W. Webb, Phys. Rev. Lett. 33 (1974) 168 T c of Nb 3 Sn after 1 MeV neutron irradiation WAMSDO 2011 Workshop (CERN), 14.11.1117

18 Recovery of Nb 3 Sn films after irradiation at T < 30K with 25 MeV O-ions (B. Besslein, 1976) < 1K WAMSDO 2011 Workshop (CERN), 14.11.1118

19 Fluence (x 10 18 n/cm 2 ) T ann (K) E > 0.1 MeV Neutron irradiation of a multifilamentary Nb 3 Sn wire, followed by an anneal of 5 min. at T ann. B.S. Brown, T.H. Blewitt, T.L. Scott, D.G. Wozniak,, J. Appl. Phys.49(1978) 4144 19 Recovery Effects after warming up WAMSDO 2011 Workshop (CERN), 14.11.1119 6 %

20 WAMSDO 2011 Workshop (CERN), 14.11.1120 Volume expansion of irradiated Nb 3 Sn

21 Analogy between neutron and heavy ion irradiation Scaling law between various sources not yet investigated WAMSDO 2011 Workshop (CERN), 14.11.1121 1x 10 18 n/cm 2  V ≈ 1% At 1 x 10 18 n/cm 2, volume expansion of Nb 3 Sn is ≈ 1%: * internal stresses? * effects on J c ?

22 a  t (x 10 19 n/cm 2 ) WAMSDO 2011 Workshop (CERN), 14.11.1122 A. Sweedler, 1978 Schneider, 1982 Volume expansion after irradiation

23 Suppression of martensitic transformation in Nb 3 Sn films irradiated with 20 MeV 32 S ions at < 30 K (2 x 10 15 cm -2 ) (C. Nölscher, 1984) Hall constant WAMSDO 2011 Workshop (CERN), 14.11.1123

24 WAMSDO 2011 Workshop (CERN), 14.11.1124 Irradiation of binary and ternary alloyed Nb 3 Sn

25 10 17 10 18 10 19 10 20 Fluence (n/cm 2 ) H.W. Weber et al., 1986, Adv. Cryo. Eng., 32, 853 J c /J co 8T 4T E > 0.1 MeV (Nb- 1.5wt.%Ti) 3 Sn wires Binary Nb 3 Sn wires 25 E > 0.1 MeV ~ 3 x 10 17 1.5 x 10 18 12T 10T 8T 4T WAMSDO 2011 Workshop (CERN), 14.11.1125

26 WAMSDO 2011 Workshop (CERN), 14.11.1126 Binary Nb 3 Sn Bronze route 10’000 filaments Binary Nb 3 Sn Bronze route 19 filaments F. Weiss, R. Flükiger, W. Maurer, P.A. Hahn, M.W. Guinan, IEEE Trans. Magn., MAG 23(1987)976 Neutron irradiation E = 14 MeV I c (max) varies for different wire configurations

27 WAMSDO 2011 Workshop (CERN), 14.11.1127 I c (max) are different for different neutron sources: When comparing the effect of irradiation for different neutron sources e.g. 1 MeV and 14 MeV, the fluences have to be considered carefully, and the appropriate corrections have to be made

28 WAMSDO 2011 Workshop (CERN), 14.11.1128 Binary Nb 3 Sn wire (19 filaments) Ti alloyed Nb 3 Sn wire (19 filaments) E = 14 MeV This effect does not depend on the neutron source, but on the Nb 3 Sn wire configuration

29 29 Behavior of J c under stress after irradiation WAMSDO 2011 Workshop (CERN), 14.11.1129

30 Stress – strain curves before and after irradiation Bronze Route multifilamentary wire T irr = 350 K 4.2 K fluence Recovery after annealing at 450 and 700 °C T. Okada, M. Fukumoto, K. Katagiri, K. Saito, H. Kodaka, H. Yoshida, IEEE Trans. Magn., MAG-23(1987)972 Hardening with higher fluence 30WAMSDO 2011 Workshop (CERN), 14.11.1130

31 Effect of uniaxial tensile strain after irradiation I c (A) I c (A) Strain (%) Strain (%) Strain (%) T. Okada, M.Fukumoto, K.Katagiri,K.Saito, H.Kodaka, H.Yoshida, IEEE Trans.Magn. MAG-23(1987)972 Bronze Route Multifilamentar y Nb 3 Sn wire Before Irradiation After Irradiation  m = 0.2%  m = 0.4% 31WAMSDO 2011 Workshop (CERN), 14.11.1131

32 WAMSDO 2011 Workshop (CERN), 14.11.1132 The effect of proton irradiation on Nb 3 Sn (thin films)

33 WAMSDO 2011 Workshop (CERN), 14.11.1133 Fluence (x 10 17 p/cm 2 ) 0.6 x 10 17 p/cm 2 I c /I co Maximum of I c after proton irradiation Binary Nb 3 Sn 0 1 2 3 4 J c max for neutrons 8 x 10 17 n/cm 2 4T – 30 GeV, Snead et al.

34 WAMSDO 2011 Workshop (CERN), 14.11.1134 Binary Nb 3 Sn wires (and films): Maximum of I c : neutrons: 8 x 10 17 n/cm 2 protons: 6 x 10 16 p/cm 2 Still necessary to know behavior after proton irradiation, in spite of 3% fluence with respect to neutrons ! Ternary Nb 3 Sn wires: Maximum of I c : neutrons: 2 x 10 17 n/cm 2 protons: ? Even more necessary: behavior under pion irradiation. Total damage of protons + pions becomes comparable to that caused by neutrons

35 WAMSDO 2011 Workshop (CERN), 14.11.1135 Planned operations at CERN C. Scheuerlein T. Spira PhD, will start January 2012 R. Flükiger L. Bottura A. Ballarino G. De Rijk Calculations: Collaboration with F. Cerutti (CERN) F. Broggi, Milano)

36 Planned operations at CERN - 1 Material: Nb 3 Sn with additives (Internal Sn, PIT) Ti Ta (activation!) Neutron irradiation, 1 MeV, Collaboration with Atominstitut Vienna Neutron irradiation of Nb 3 Sn wires at 1 MeV and 14 MeV has already been performed 20 years ago However, new investigation on high J c wires with precisely determined neutron fluence at 300K (see the presentation of Harald Weber) WAMSDO 2011 Workshop (CERN), 14.11.1136

37 1: Confirm the systematic difference between binary and ternary alloyed Nb 3 Sn wires after neutron irradiation 2: Establish the maximum of J c vs. fluence; find out at which fluence the values of J c and H c2 2: Comparison between resistive and inductive J c measurements on Internal Sn and PIT wires T. Baumgartner et al., MT22 (H. Weber’s talk) Advantage: once the scaling is established, J c can be determined on 3 mm wire pieces by magnetization. This result will be used for measuring J c in proton irradiated wires Goal of the collaboration with Atominstitut Vienna: WAMSDO 2011 Workshop (CERN), 14.11.1137

38 Planned operations at CERN - 2 Proton Irradiation at various energies Material: Nb 3 Sn Internal Sn and PIT wires, with Ta and Ti additives Collaborations with: * Kurchatov Institute (Russia)35 MeV10 18 p/cm 2 * Université catholique, 65 MeV10 17 p/cm 2 Louvain la Neuve, Belgique * CERN: IRRAD124 GeV10 17 p/cm 2 ISOLDE1.4 GeV10 18 p/cm 2 First magnetization measurements of wires after decay: after mid 2012 WAMSDO 2011 Workshop (CERN), 14.11.1138

39 Proton irradiations at Kurchatov Institute: Program Duration : 24 months Proton energy: 35 MeV Temperature: 300K (+ heating due to proton impact) Maximum fluence:1x 10 18 p/cm 2 Tasks on irradiated wires:J c by magnetization measurements*)**) Electrical resistivity vs. T T c TEM Lattice parameters Tasks on irradiated bulks: Long range atomic order parameter*) Calculations: dpa calculations for proton irradiation *) Measurements will be performed at CERN **) Transport J c on proton irradiated wires: will be done later WAMSDO 2011 Workshop (CERN), 14.11.1139

40 WAMSDO 2011 Workshop (CERN), 14.11.1140 Conclusions (superconductors) We are still at the beginning of our investigations: *Need for proton and pion irradiations of Nb 3 Sn wires *Are binary or ternary alloyed Nb 3 Sn wires better? *How has the volume expansion (1% at 10 18 n/cm 2 ) to be taken into account? *Irradiations at 4.2K still necessary (very small number, for comparison) *Warming up and cooling cycles needed for reliability tests *New devices for testing at 15 T needed *New devices for mechanical testing needed *Calculations needed: dpa, but also combined irradiations

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