a magnetic refrigeration stage

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Presentation transcript:

a magnetic refrigeration stage 26/04/2017 Study of a magnetic refrigeration stage Francois Millet – March 2015

Magnetic refrigeration principles Review of the state-of-the-art Contents Motivations Magnetic refrigeration principles Review of the state-of-the-art Preliminary design study Conclusions

FCC Cryogenic Requirements Superfluid Helium cooling for : High-field superconducting magnets of FCC-hh (10 kW range at 1.8 K) High-gradient superconducting RF cavities of FCC-ee (5 kW range down to 1.6 K) L. Tavian / CERN FCC cryogenic requirements : Large superfluid refrigeration capacity with high efficiency & high reliability E.Palmieri / INFN x 4.4 x 1.6 E.Jensen / CERN

Superfluid Helium Refrigeration Existing large HeII refrigeration use cold compressor in series Complex control strategy Long downtime after stops Limited Carnot efficiency < 20 % Is there any option for a more efficient and more reliable solution ? “Integral cold” cycle “Mixed” cycle” CEBAF - SNS LHC Generic scheme of < 2 K refrigeration cycles L.Tavian/ CERN

Magnetic Refrigeration Option Magnetic refrigeration stage More reliable ? Cold compressors could be totally or partially replaced by a Magnetic Refrigeration stage 300 K to 4.5 K refrigeration More efficient ? High Carnot efficiency (> 50%) already measured at low cooling capacity for Magnetic Refrigeration stage between 1.8 K and 4.2 K 4.5 K helium Magnetic refrigeration stage 1.8 K helium Heat load Qc

Contents Motivations Magnetic refrigeration principles Review of the state-of-the-art Preliminary design Study Conclusions

Magnetic Refrigeration principles Magnetic Refrigeration or Adiabatic Demagnetization Refrigeration (ADR) is a cyclic cooling system which alternates between two states : Operating state : Cool-down and heat removal from the cold source (Qc) Recycling state : Warm-up and heat rejection to the warm source (Qw) Warm source Thermal load Qw Magnetic refrigeration stage Magnetisation / Demagnetisation Thermal load Qc Cold source

Magneto Caloric Effect Magnetic refrigeration is based on the Magneto-Caloric Effect (MCE) (reversible variation of internal energy when applied magnetic field in a suitable material) 𝑀𝐶𝐸= 𝜕𝑇 𝜕𝐵 𝑆 Apply magnetic field spins align temperature increases Remove magnetic field spins randomize temperature decreases Magneto Caloric Effect was discovered in pure iron in 1881 by Emil Warburg The cooling technology was first demonstrated experimentally in 1933 by William F. Giauque & D.P. MacDougall (< 1 K) IFW Dresden

Contents Motivations Magnetic refrigeration principles Review of the state-of-the-art Preliminary design Study Conclusions

Worldwide works in magnetic refrigeration Sub-kelvin application (space detectors & laboratory cooling) Efficient & reliable products (space-qualified) 1 to 4.5 K cooling (LTS magnets & space detectors) Laboratory prototypes with achieved high efficiency 20-77 K range (Hydrogen liquefaction) On-going R&D Room temperature application Space-qualified 50 mK cooler (CEA/SBT)

=> Carnot efficiency > 50 % CEA works Reciprocating magnetic refrigeration between 1.8 K and 4.2 K (A.Lacaze & al., Double acting reciprocating magnetic refrigerator : recent improvements, 1984) Magnetic material (GGG) Warm source (4.2 K) Liquid He Cold source 1.8 K 2.1 K Useful power Qc 1.35 W 2.2 W FOM 53% 79,3% Frequency 0.8 Hz 0.6 Hz Magnetic field 4 T (stationary) Magnetic material GGG (moving) 0.1 kg Heat transfer Alternatively in HeI & Pressurised HeII Warm source 4.2 K Moving magnetic material Stationary magnetic field Alternatively heat transfer in Liquid HeI or Pressurised HeII Stationary magnets Cold source (1.8 K) Pressurized He II => Carnot efficiency > 50 %

=> Innovative solutions for heat transfer Hitachi works Magnetic refrigeration between 1.8 K and 4.2 K (Y.Hakuraku & al., Thermodynamic analysis of a magnetic refrigerator with static heat switches, 1986) (Y.Hakuraku & al., A Rotary Magnetic Refrigerator for Superfluid Helium Production, 1986) Warm source (4.2 K) Liquid He Static design / Rotating design Cold source 1.8 K Useful power 1.5 W 1.8 W FOM 20% 34% Frequency 0.2 Hz 0.4 Hz Magnetic field 3 T (pulsed) 3 T (station.) Mag. material GGG (static) GGG (rota.) 1.1 kg Heat transfer Permanent in HeI & HeII Alternatively in HeI or HeII Warm source 4.2 K Pulsed magnets Static magnetic material, Pulsed magnetic element Static heat switches (Boiling in Liquid He I and condensation of He II gas) Rotating magnetic material, Steady magnetic element Cycling heat transfer with HeI and He II baths Boiling heat transfer Magnetic material (GGG) condensation heat transfer Gaseous helium Cold source (1.8 K) Saturated He II => Innovative solutions for heat transfer Hakuraku / Hitachi

Magnetic Refrigeration between 1.8 K and 4.2 K CERN works Magnetic Refrigeration between 1.8 K and 4.2 K (A.Bezaguet & al., Design and construction of a static magnetic refrigeration between 1.8 K and 4.5 K, 1994) Cold source 1.8 K Useful power 10 W (first tests) FOM ~10% (estimate) Frequency 0.2 to 1 Hz Magnetic field 3,5 T (pulsed) Magnetic material GGG (static) 10 kg Heat transfer Alternatively He I or He II flow circulation Warm source 4.2 K Static magnetic material, Pulsed magnetic field Oscillating flow circulation from HeI bath or HeII pressurised bath Works performed during the LHC preparatory phase but stopped just after first tests ! M.Schmidt / CERN

Tandem Magnetic Regenerative Refrigeration between 1.8K-4.2K MIT works Tandem Magnetic Regenerative Refrigeration between 1.8K-4.2K (S.Jeong & al., Experimental investigation of the regenerative magnetic refrigerator for 1.8 K, 1994) Cold source 1.8 K Useful power 19 mW FOM ~10% (estimate) Frequency 0.07 Hz Magnetic field 2.8 T (pulsed) Magnetic material GGG (static) 0.135 kg Heat transfer Oscillating He3 (60 mbar) Warm source 4.2 K Static magnetic material, Pulsed magnetic field Oscillating Flow circulation => Tandem operation with He3 oscillating flow S.Jeong / MIT

Contents Motivations Magnetic refrigeration principles Review of the state-of-the-art Preliminary Design Study Conclusions

Perspectives from the state-of-the-art Favorable operating temperature range < 5 K with high efficiency MCE High achieved efficiency > 50% at 1.8 K Various design options stationnary or pulsed magnet field, conduction or convection heat transfer => Need to select a design option and to scale up towards 1 to 10 kW at 1.8 K or 5 kW down to 1.6 K Strong CEA experience in magnetic refrigeration at subkelvin temperature for space cooling (heat switch, heat transfer, paramagnetic material development) Space-qualified 50 mK cooler

Key parameters selection Objectives FCC-ee : up to 5 kW down to 1.6 K (J/kg.mol) Magnetic Material ? Selection of GGG for first iteration Gadolinium Gallium Garnet Gd3Ga5O12 Thermodynamic cycle & Magnetic Field ? 2.1 K 4.5 K 1.6 K Selection of Magnetic Carnot cycle 4 T at 4.5 K or 2 T at 2.1 K Up to 55 dm3 per kW at 1.6 K / 0,1 Hz Heat exchange ? GGG volume = f(Qc,f,Twarm,B) Helium flow circulation

First iteration on design and simulations Preliminary design First iteration on design and simulations Cold source 1.6 K Useful power Objectives : up to 5 kW FOM Objectives : > 50% Frequency 0.1 Hz Magnetic field 4 T Magnetic material GGG Heat transfer Oscillating He Warm source 4.2 K Adiabatic Magnetization & Demagnetization Flow Magnetization & Demagnetization Work started in the framework of FCC collaboration

Contents Motivations Magnetic refrigeration principles Review of the state-of-the-art Preliminary design Study Conclusions

Conclusions Large superfluid helium refrigeration capacity is required for the FCC project 10 kW range at 1.8 K for FCC-hh & 5 kW-range down to 1.6 K for FCC-ee Magnetic refrigeration as alternative option to conventional gas cycles in terms of efficiency and reliability no or few cold compressors for helium bath pumping > 50% Carnot efficiency expected according to prototypes results Key parameters for a magnetic refrigeration stage have been selected and a preliminary design is on-going Challenging design study started at CEA in 2015

Thanks you for your attention Any question ?