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Outline of Lecture 2 Thermo modynami mics and ph phase More on the theory of tricritical transitions (see blackboard) transitions in ma magnetic ma materials An introduction to magnetic cooling (to be continued in Lecture 3) Lec


  1. Outline of Lecture 2 Thermo modynami mics and ph phase • More on the theory of tricritical transitions (see blackboard) transitions in ma magnetic ma materials • An introduction to magnetic cooling (to be continued in Lecture 3) Lec Lectur ure 2 e 2 Karl G. Sandeman ESM 2013 Critical exponents: experiment vs theory for d =3 More comparisons Ising X-Y Heisenberg d=1 No ordering! No ordering! No ordering! d=2 β =1/8; γ =7/4 Special No ordering! case! d=3 β =0.32; γ =1 β =0.35; γ =1 β =0.36; γ =1.39 Mean field β =1/2; γ =1 Here “ t ” is proportional to T-T c Table from Ben Simons’ lectures on Phase Transitions and Collective Phenomena, U. Cambridge.

  2. A phase diagram of the Ginzburg-Landau Hamiltonian CoMnSi: imaging tricriticality using a Hall probe CoMnSi 0.92 Ge 0.08 Antiferromagnet to high-magnetisation state, induced by field Low T: - 1st order - Globally “continuous” - Locally sharp, hysteretic High T: - 2nd order - Globally and locally continuous - No hysteresis This diagram is from Ben Simons’ lectures on Phase Transitions and Collective Phenomena, U. Cambridge. Morrison et al., Phys. Rev. B (2009) Vapour compression refrigeration Solid-state cooling at room temperature Refrigerant Critical Critical temp. pressure CO 2 31 ˚C 7.38 MPa Ferroic cooling, R22 96.2 ˚C 4.99 MPa R134a 101 ˚C 4.06 MPa including magnetic cooling The efficiency of the refrigerant is directly related to the critical Gas compression refrigeration temperature. works in sub-critical regime Tuning the critical point and the pressure-temperature phase line gradient are very important

  3. Magnetic refrigeration: a growing area of interest Magnetic cooling: the future m = l ∑ ∑ m ( H M ) d ( Y l m ( Ω M )) dG = − SdT − MdH M + K l + Vdp + ... A careful system-wide cost and efficiency analysis revealed the benefit of l m = − l magnetic cooling at low powers (< 500 Watt). A research frontier Magnetocaloric principles Can also be described in terms of isothermal entropy change , Δ S: Energy efficiency Rare earth Apply magnetic field metal use H $ ' ∂ M ( T ', H ') adiabatically ∫ Δ S total ( H , T ) = dH ' & ) % ∂ T ' ( 0 H ' S total =S magnetic + S lattice + S electronic Maxwell relation for continuous M(T,H) Magnetic cooling S magnetic high S magnetic low S lattice low S lattice high Δ S total ( H , T ) = −Δ M dH c dT Δ T ad ( H , T ) = T Δ S Clausius-Clapeyron eqn. for 1st order C p transition in M Magnetic phase HFC-free cooling transition physics So the material (usually) heats in an applied field ( Δ T ad >0) The effect is maximal at a (magnetic) phase transition The sign of (dM/dT) is crucial and yields two possibilities for the MCE

  4. Magnetocaloric benchmark material at RT: Gd The cycle K-type thermocouple A d i a b a t i c M a g n e t o c a l o r i c E f f e c t i n G d ( 0 - 2 T ) 5 Temperature Change (˚C) Gd 4 3 2 1 magnetic field 0 - 2 0 - 1 0 0 1 0 2 0 3 0 4 0 T e m p e r a t u r e ( D e g r e e s C ) K. G. Sandeman, Mag. Tech. Int. 1 30-32 (2011) � Magnetocaloric principles State of the art (2010) Inverse Inverse M M Lists 41 prototypes to 2010. Most used Gd as refrigerant at that time. No clear example of end-user integration at that time. The situation has already changed in the 3 years since… T c T T t T c T

  5. What makes a good magnetic refrigerant? Single phase refrigerants A candidate magnetic refrigerant at room temperature: La(Fe,Si) 13 Cheap MnFe(P,Z) d-metal magnetism La(Fe,Co,Mn,Si) 13 ~11.6 Å First order transition Δ T ad ( H , T ) = T Δ S because ∆ T ad of second order transtion is too low (if d-metal C p alloy) 2 nd H Proximity to (tri)critical point order Minimise energy loss from hysteresis 1 st order ∂ H of phase line is also important (see next) T C ∂ T T La(Fe,Si) 13 cubic crystal structure Fujita et al., 2003 Tuning transition temperature La-Fe-Co-Si La-Fe-Mn-Si-H 14,0 x = 0.050 y=0.390 x = 0.058 y=0.373 10,00 y=0.356 x = 0.065 12,0 y=0.338 x = 0.075 y=0.322 8,00 x = 0.087 10,0 x = 0.099 - Δ S m (Jkg -1 K -1 ) - Δ S m (J/kgK) x = 0.112 8,0 6,00 Gd 6,0 4,00 4,0 2,00 2,0 0,00 0,0 -30,0 -20,0 -10,0 0,0 10,0 20,0 30,0 40,0 50,0 60,0 70,0 80,0 270 280 290 300 310 T (°C) Temperature (K) Magnetic entropy change as a function of temperature of: La(Fe 0.915 Co x Si 0.085 ) 13 ( left ) and five LaFe 11.74-y Mn y Si 1.26 H 1.53 alloys with different y ( right ) for a magnetic field change of 1.6 T. The entropy change is higher than that seen in gadolinium (Gd, left plot only).

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