Magnetic
refrigeration (MR), which offers considerable operating cost savings
by eliminating the most inefficient part of the refrigerator -- the
compressor -- is rapidly becoming competitive with conventional gas
compression technology. In addition, MR offers two important
environmental benefits: because of its reduced energy consumption,
the amount of greenhouse gases produced by fossil fuel power plants
is reduced; and a major source of ozone depleting
chlorofluorocarbons (CFCs) is eliminated because solid magnetic
materials are used as the cooling agents, and water (or antifreeze)
or gaseous helium as the heat transfer medium. Recent developments
in MR design by the Ames Laboratory and the Astronautics Corporation
of America plus the discovery of a new family of giant
magnetocaloric effect materials, could soon bring the potential for
widespread commercialization of magnetic refrigeration technology
close to realization.
Magnetic refrigeration is based on the magnetocaloric effect
(MCE), an intrinsic property of all magnetic materials that peaks in
the vicinity of the magnetic ordering temperature. In the case of a
ferromagnetic material, it is the warming as the magnetic moments of
the atoms are aligned on the application of a magnetic field, and
the cooling when the magnetic moments become randomly oriented on
removing the magnetic field. The warming and the cooling of a
magnetic material in response to a changing magnetic field is
similar to the warming and the cooling of a gaseous medium in
response to compression and expansion. Therefore, MR operates by
magnetizing/demagnetizing the magnetic material.
Since the refrigerant is a solid (usually spheres or thin
sheets), the heat transfer is provided by a fluid, such as water,
water containing antifreeze, or an inert gas, depending on the
operating temperature. This replaces the compressor and the gas or
the low boiling temperature liquid in conventional refrigeration
systems. However, the controlling circuits remain essentially the
same.
A schematic of the successful laboratory magnetic refrigerator
for near room temperature applications, built by the Astronautics
Corporation of America in collaboration with the Ames Laboratory, is
shown in Figure 1. The magnetic field is provided by a conventional
liquid helium-immersed superconducting niobium titanium (NbTi)
solenoid mounted in a Dewar container with a warm bore (a
cylindrical opening along the central axis that stays at room
temperature). The magnet is run in the persistent mode (i.e. the
current continues to flow inside the closed superconducting loop in
the absence of an external current source). The refrigerant is the
pure lanthanide metal, gadolinium (Gd), which orders
ferromagnetically at 21° C (294 K). The two
regenerator beds are composed of Gd spheres (a total of 1.5 kg in
each bed) that are mounted on a carrier assembly, and alternately
inserted in the bore of the magnet using an air cylinder drive. The
drive movement takes 1 s.
The magnetized bed inside the magnet is warmed due to the
magnetocaloric effect (MCE), and the demagnetized bed outside the
magnet is cooled due to the reverse MCE. The heat transfer fluid in
this MR is water, which is pumped through the beds and heat
exchangers as shown in the diagram. The water picks up heat when
passing through the magnetized (hot) bed cooling the Gd inside, and
then the heat is dissipated as the water passes through the hot heat
exchanger. The heat load is picked up by the water in the cold heat
exchanger and is dissipated when passing through the demagnetized
(cold) bed warming the Gd inside. The flow is accomplished in
approximately 2 s, after which the positions of the beds are
interchanged (i.e. the previously demagnetized bed is inserted
inside the magnet and the previously magnetized bed is on the
outside). The flow of the water is rerouted accordingly and the
refrigeration cycle is repeated.
The experimental results of the energy efficiency of this MR
system are depicted in Figure 2. The Carnot efficiency has been
calculated excluding the energy losses in the seals, which in this
refrigerator were standard off-the-shelf seals. The use of special
low friction seals would greatly reduce these losses. As can be
seen, the efficiency of this MR is about the same order of magnitude
as for commercial vapor cycle refrigerators (20 to 30% of Carnot),
even at the lowest magnetic field change from 0 to 1.5 T. It reaches
50 to 60% when the magnetic field increases to 5 T.
The overall cooling power that has been obtained ranges from 200
W to 600 W, depending on the magnetic field strength and other
operating parameters. From the total volume of the two beds packed
with the magnetic refrigerant, which is just under 600 ml, the
specific cooling power obtained is about 1 W/ml. The observed
coefficient of performance (COP), which is defined as the ratio of
cooling power to work input, ranges from 2 to 9. This compares
favorably with the COP observed for most standard gas compression
devices.
The maximum magnetocaloric effect (MCE) in Gd occurs at the
temperature where it orders ferromagnetically (294 K or 21° C). When the magnetic field changes from 0 to
1.5 T, its MCE (i.e. the change in its temperature when the magnetic
field changes) is 4.5 K (or 4.5° C), and 11
K (or 11° C) when the magnetic field
changes from 0 to 5 T. Nonetheless, as shown on Figure 2, the
temperature span achieved exceeds the maximum MCE by a factor of 2
to 3 at a competitive efficiency. This is made possible by using an
unusual thermodynamic cycle –- active magnetic regeneration (AMR)--
in which the magnetic refrigerant acts both as a refrigerant and a
regenerator. Clearly, the performance of this MR would be enhanced
by using a magnetic refrigerant material with a larger MCE than Gd
as well as by improving the refrigerator’s design.
Intermetallic alloys recently discovered at the Ames Laboratory
provide these much improved magnetic refrigerants. They are formed
in the ternary system gadolinium-silicon-germanium (Gd-Si-Ge), and
their stoichiometry,
Gd5(SixGe1-x)4,
corresponds to the pseudobinary cross-section
Gd5Si4 - Gd5Ge4. The
zero magnetic field phase diagram of this system is shown in Figure
3. The alloys with 0.5 < x £ 1, i.e. the Si- rich
Gd5Si4-based solid solution, are normal
ferromagnets. The Gd5Ge4-based solid solution
extends from 0 £ x £ 0.2. The two-step magnetic ordering
occurs in this region with the upper transition being from a
paramagnet (average alignment of magnetic moments close to random)
to a ferrimagnet (partial anti-parallel alignment of magnetic
moments), and the lower one from a ferrimagnet to a ferromagnet
(parallel alignment of magnetic moments). The upper ordering
temperature in the alloys with 0 £
x £ 0.2 is almost
independent of composition, while the lower transition temperature
decreases rapidly as x goes from 0.2 to 0.
The intermediate ternary solid solution phase
Gd5(SixGe1-x)4 extends
from 0.24 £ x £ 0.5 and has a monoclinically distorted
lattice, derived from the parent orthorhombic samarium germanium
(Sm5Ge4) type structure formed by both
Gd5Si4 and Gd5Ge4. The
alloys in this phase region also order magnetically in two steps: on
lowering the temperature they initially order ferromagnetically, and
at a slightly lower temperature they undergo a second transition
from ferromagnet-I to ferromagnet-II. For all of the alloys with
x £ 0.5 the upper transition is
a second order transition and the lower one is a first order phase
transition. The bulk of the magnetic entropy is associated with the
lower temperature first order phase transition. This brings about a
magnetocaloric effect, which can also be expressed in terms of the
magnetic entropy change, D Smag,
exceeding that of previously known lanthanide metals and alloys by a
factor of 2 to 7, as shown on Figure 4.
The Gd5(Si2Ge2) alloy represents
the terminal composition where the magnetic properties change
abruptly on further increase of the silicon content (see Figure
3).
The lower ordering temperature for this alloy is 276 K (3° C), and the giant magnetocaloric effect extends
to just above 290 K (17° C) for a
magnetic field change from 0 to 5 T. This alloy would make an
excellent refrigerant material for a refrigerator with the heat
rejected into chilled water. However, for use in a magnetic
refrigerator with the heat rejection into the ambient environment
(i.e. the temperature of the hot sink would be approximately equal
to 25-35oC, or 298-308 K) one needs a material with an
ordering temperature greater than 276 K. By alloying
Gd5(Si2Ge2) with trivalent gallium
(Ga) substituting for the mixture of tetravalent Si+Ge its
properties can be selectively modified.
The more metallic nature of Ga most likely affects the
distribution of electrons between the valence and conduction bands,
and the small alloying addition of Ga (0.333 at.%) retains the
monoclinic crystal structure, which is necessary to preserve the
first order magnetic phase transition and to maintain the giant
magnetocaloric effect. Simultaneously, it probably enhances the
exchange interactions which causes the increase of both the upper
and the lower ordering temperatures in the
Gd5(Si1.985Ge1.985Ga0.03)
alloy. In fact, the lower (first order phase transition) occurs at
~ 286 K (13° C), and the 0 to 5 T magnetic field change
extends the region of the giant magnetocaloric effect from ~ 290 (17° C ) to
310 K (37° C), as shown in Figure 4.
Another important parameter characterizing the potential for the
use of magnetic refrigerants is the refrigerant capacity, which is
defined as:
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where T1 and T2 are the temperatures of the
hot and cold sinks, respectively, and D
Smag (T) is the refrigerant’s magnetic entropy change as
a function of temperature. The refrigerant capacity, therefore, is a
measure of how much heat can be transferred between the cold and hot
sinks in one ideal refrigeration cycle. A comparison, shown in
Figure 5, of some of the
Gd5(SixGe1-x)4 alloys
with the best known refrigerants in the corresponding ranges of
temperature shows that the new materials have 25 to 120% more
capacity than any known magnetic refrigerant. This should translate
into a corresponding increase in the MR performance provided that
all other key factors, such as the MR design and the heat transfer
characteristics, are unchanged.
The Gd5(SixGe1-x)4
series of alloys, where 0 £
x £ 0.5, plus the
Gd5(Si1.985Ge1.985Ga0.03)
alloy have an extremely large magnetocaloric effect exceeding that
in known prototypes by as much as a factor of 2 (in terms of
refrigerant capacity) and by a factor of 7 (in terms of D Smag). Another unique feature of
this series of materials is that the magnetic ordering temperature
where the giant magnetocaloric effect exists can be easily tuned
between room temperature and the liquefaction temperature of
hydrogen gas. Therefore, the discovery of the large magnetic cooling
capacity of the
Gd5(Si1-xGex)4
materials, combined with the successful design of the laboratory
scale magnetic refrigerator, offer the long awaited breakthroughs in
active magnetic regenerator magnetic refrigeration technology. It is
anticipated that the widespread commercialization of this cooling
technology will take place in time to provide large benefits in
energy savings, in the reduction of greenhouse gases, and in the
preservation of the environment.
At the present stage of magnetic refrigeration technology
expanded support from industry and government would make possible a
rapid transition from the laboratory scale (proof of the principle)
refrigerator to commercially assembled, highly efficient and
reliable magnetic refrigerator units. Magnetic refrigeration is
unique because it is potentially scaleable in size and power (from
Watts to MegaWatts of cooling power near room temperature)
without significant losses in efficiency. In contrast,
scaling down is intrinsically difficult with conventional gas
compression technology. Government and industrial support is
necessary to continue studies of the basic phenomena related to the
magnetocaloric effect, and the engineering fundamentals of the
performance of new laboratory scale magnetic refrigerators powered
by either superconducting or permanent magnets. New laboratory scale
magnetic refrigerator units employing different designs need to be
built and comprehensively tested with known and new magnetic
refrigerant materials. This will result in an understanding of the
fundamental relations between composition, crystal, and magnetic
structures, and the magnetothermal properties of solid magnetic
materials; and also the behavior of magnetic materials in an
environment of varying magnetic fields. The ultimate goal is the
design of better magnetic refrigerants and more energy efficient
magnetic refrigerators.
Iowa State University holds several materials patents including
the one on the giant magnetocaloric effect materials. Astronautics
Corporation of America holds several patents involving magnetic
refrigeration devices, and additional ones are being sought. Both
organizations are continuing development efforts, and welcome
inquiries from industry about joint development of this
technology.
Karl A. Gschneidner, Jr., Ph.D., Ames Laboratory,
Iowa State University, Ames, IA 50011-3020.
Phone: (515)-294-7931
Fax: (515)-294-9579
E-mail: CAGEY@ameslab.gov
Vitalij K. Pecharsky, Ph.D., Ames Laboratory,
Phone: (515)-294-8220. Fax: (515)-294-9579. E-mail: VITKP@ameslab.gov
For the devices: Carl B. Zimm, Astronautics
Corporation of America, Astronautics Technology Center, 5800 Cottage
Grove Rd., Madison, WI 53716. Phone: (608)-221-9001. Fax:
(608)-221-9104. E-mail: ZIMM%astroatc.UUCP@cs.wisc.edu