Frustrated magnet for adiabatic demagnetization cooling to milli-Kelvin temperatures
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https://doi.org/10.1038/s43246-021-00142-1
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Frustrated magnet for adiabatic demagnetization
cooling to milli-Kelvin temperatures
1234567890():,;
Yoshifumi Tokiwa
Philipp Gegenwart
1,2 ✉, Sebastian Bachus1, Kavita Kavita1, Anton Jesche
1, Alexander A. Tsirlin1 &
1
Generation of very low temperatures has been crucially important for applications and fundamental research, as low-temperature quantum coherence enables operation of quantum
computers and formation of exotic quantum states, such as superfluidity and superconductivity. One of the major techniques to reach milli-Kelvin temperatures is adiabatic
demagnetization refrigeration. This method uses almost non-interacting magnetic moments
of paramagnetic salts where large distances suppress interactions between the moments.
The large spatial separations are facilitated by water molecules, with a drawback of reduced
stability of the material. Here, we show that the water-free frustrated magnet KBaYb(BO3)2
can be ideal for refrigeration, achieving at least 22 mK. Compared to conventional refrigerants, KBaYb(BO3)2 does not degrade even under high temperatures and ultra-high vacuum.
Further, its magnetic frustration and structural randomness enable cooling to temperatures
several times lower than the energy scale of magnetic interactions, which is the main limiting
factor for the base temperature of conventional refrigerants.
1 Experimental Physics VI, Center for Electronic Correlations and Magnetism, University of Augsburg, Augsburg, Germany. 2 Advanced Science Research
Center, Japan Atomic Energy Agency, Tokai, Ibaraki, Japan. ✉email:
COMMUNICATIONS MATERIALS | (2021)2:42 | https://doi.org/10.1038/s43246-021-00142-1 | www.nature.com/commsmat
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COMMUNICATIONS MATERIALS | https://doi.org/10.1038/s43246-021-00142-1
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uppression of thermal fluctuations by lowering temperature
gives access to intricate and potentially usable quantum
effects. Major discoveries, such as the quantum Hall effect
and superfluidity and superconductivity, have been made by
explorations of matter close to absolute zero1,2. Recently, the
development of quantum computers and sensors for dark matter
detection rendered low-temperature refrigeration an important
technological challenge3,4. One of the viable methods for reaching
the milli-K (mK) temperature range is adiabatic demagnetization
refrigeration (ADR) using paramagnetic salts5–7. Its main
advantages over the currently dominant technique, 3He–4He
dilution refrigeration, are the simple construction of a cooling
device and its operation without the usage of expensive 3He. The
recent crisis of 3He, which was caused by the increased demand
due to the construction of neutron detectors for defense against
nuclear terrorism, raised serious concerns about the strong
dependence of the current technology on such a scarcely available
and ever more expensive gas8–10. This triggered renewed interest
in ADR, as well as interesting proposals of completely new types
of ADR materials11–19.
The only advantage of 3He–4He dilution refrigeration is its
capability of continuous cooling while conventional ADR is a
single-shot technique. This makes the 3He–4He dilution refrigeration more commonly used than ADR. However, the situation
may change thanks to recent developments of continuous ADR
cooling20,21 and the availability of commercial continuous
refrigerators based on ADR22. Therefore, ADR has the potential
of becoming the main cooling technology already in near future,
at least in the mK temperature range.
ADR uses magnetic moments of almost-ideal paramagnets
with very weak magnetic interaction J . Because the interaction is
weak, magnetic moments are easily aligned by the external
magnetic field, causing a reduction of entropy (Fig. 1a, b). Even at
zero external magnetic field H = 0, magnetic moments of such
almost-ideal paramagnets experience some small internal magnetic field produced by adjacent magnetic moments through
magnetic interactions. This causes a tiny Zeeman splitting and
magnetic order at the same energy scale ( Δ0 J ). Therefore,
entropy, which is the driving force of ADR, decreases to zero
below the temperature of T J , thus putting a limit on the end
temperature T f J that can be reached via ADR with this
material (Fig. 1b). As indicated by a black horizontal arrow in
Fig. 1b, the entropy difference between H = 0 and H ≠ 0 is the key
for ADR. While a perfect paramagnet with zero magnetic interactions would be an ideal refrigerant, having maximum entropy
at zero fields down to zero temperature, there are always weak but
finite interactions in real materials.
For many decades ever since Debye6 and Giauque7 independently proposed ADR, water-containing paramagnetic salts have
been materials of choice for cooling in the mK range5,23,24. In
these materials, the interactions are reduced by large distances
between the magnetic ions, which are separated by water molecules. However, an abundance of water makes these salts prone to
decomposition. They deliquesce in a humid atmosphere and
dehydrate in vacuum or upon even mild heating. Therefore, for
repeated use without degradation, stable water-free materials with
very weak magnetic interactions are desirable. Furthermore, ADR
would be certainly beneficial for applications in ultra-highvacuum (UHV) apparatus, especially in scanning tunneling
microscopy and angle-resolved photoemission spectroscopy
where the necessity of chamber baking at high temperature and
high vacuum for reaching UHV makes the use of current ADR
materials essentially impossible. It is, therefore, desirable to find
suitable ADR materials without water molecules.
One promising candidate for H2O-free refrigerant is KBaYb
(BO3)2 with magnetic Yb3+ ions. At sufficiently low
2
Fig. 1 Adiabatic demagnetization refrigeration. a Cooling process of a
conventional paramagnet (left) and a frustrated magnet with impeded
magnetic order (right). Green ovals represent singlet pairings in a shortrange correlated but long-range disordered state, such as a spin liquid
caused by magnetic frustration25,33 or a random-singlet state caused by
structural disorder34. b Entropy curves at zero and a finite magnetic field as
a function of temperature for conventional paramagnets (black) and a
system with suppressed magnetic order (red). While the former orders
below some temperature Tm around Δ0, or J , the latter remains disordered
down to much lower temperatures where Δ0 is an energy level splitting at
zero external fields because of the internal field caused by magnetic
interaction, J . For simplicity, a Schottky-type increase in entropy is
assumed. Note, however, that the entropy increase may be much slower in
a spin liquid because of its broad energy spectrum. Arrows with red and
black dotted lines represent cooling processes for the conventional
paramagnets (black) and frustrated magnets (red). c Crystal structure of
KBaYb(BO3)2 with triangular layers of the Yb3+ ions. Black solid (...truncated)