[TECHNICAL FIELD]
[0001] The present disclosure relates to a rare earth magnet and a production method thereof.
The present disclosure relates to a rare earth magnet containing a magnetic phase
having a composition represented by RT
5 (R is a rare earth element, and T is a transition metal element), and a production
method thereof.
[BACKGROUND ART]
[0002] Application of a permanent magnet is extended to a wide range of fields including
electronics, information communication, medical care, machine tool field, industrial
and automotive motors, etc. In addition, a requirement for reduction of carbon dioxide
emission is increasing and due to, for example, spread of a hybrid car and energy
saving in the industrial field as well as enhancement of power generation efficiency,
it has been expected in recent years that a permanent magnet having higher properties
be developed.
[0003] At present, an Nd-Fe-B magnet dominating the market as a high-performance magnet
is used also as a drive motor magnet for HV/EHV. In response to the current trend
of pursuing further size reduction and higher output of a motor, development of a
new permanent magnet material is advancing.
[0004] As one of development of a material having a performance surpassing the Nd-Fe-B magnet,
studies are being made on a rare earth magnet in which the magnetic phase is of a
binary system of a rare earth element and a transition metal element.
[0005] For example, Patent Document 1 discloses a rare earth magnet having a composition
represented by R(Fe
(1-p)Co
p)
qA
r (wherein R is one or more of Sm and Ce, 0.1≤p≤0.6, 4≤q≤6, and 0.1<r<1.0), having
a main phase of hexagonal CaCu
5 structure, and having an interstitial atom.
[CITATION LIST]
[PATENT LITERATURE]
[0006] [Patent Literature 1] Japanese Unexamined Patent Publication) No.
H4-371556
[SUMMARY OF INVENTION]
[TECHNICAL PROBLEM]
[0007] As to the binary system of a rare earth element and a transition metal element, magnetic
phases in which the molar ratio of a rare earth element and a transition metal element
is 1:2, 1:5, 1:12, 2:7, 2:17, etc. are known. In the following description, these
magnetic phases are sometimes referred to as 1-2 phase, 1-5 phase, 1-12 phase, 2-7
phase, 2-17 phase, etc., respectively.
[0008] In the binary system of a rare earth element and a transition metal element, it is
known that when the rare earth element is Sm and the transition metal element is Co,
1-5 phase is thermally more stable than 1-2 phase, 1-12 phase, 2-7 phase and 2-17
phase. Accordingly, a rare earth magnet containing Sm and Co contains a lot of SmCo
5 phases.
[0009] Since Sm is high in rarity among rare earth elements, it is attempted to replace
part or whole of Sm with a rare earth element lower in rarity than Sm.
[0010] In the rare earth magnet disclosed in Patent Document 1, at least part of Sm is replaced
with Ce. However, (Sm, Ce)Co
5 is lower in saturation magnetization than SmCo
5. In order to compensate for saturation magnetization reduced by substitution of Sm
with Ce, at least part of Co is replaced with Fe. However, when Co is replaced with
Fe, (Sm, Ce)(Co, Fe)
5 becomes extremely unstable, compared to (Sm, Ce)Co
5. As a result, the content of 1-5 phase represented by (Sm, Ce)(Co, Fe)
5 in the rare earth magnet decreases significantly, and the content of 1-2 phase represented
by (Sm, Ce)(Co, Fe)
2 increases significantly. From these fact, both saturation magnetization and anisotropy
field are reduced. Accordingly, in the rare earth magnet of Patent Document 1, even
when at last part of Co is replaced with Fe, in order to stabilize 1-5 phase, C and
N are introduced as interstitial atoms into 1-5 phase.
[0011] However, it is difficult to introduce C and N into the core part of 1-5 phase, and
therefore, it is difficult to stabilize 1-5 phase in the entire rare earth magnet.
In addition, 1-5 phase having introduced thereinto C and N is readily decomposed at
400°C or more, and thus high-temperature stability is poor.
[0012] From these facts, the present inventors have uncovered a problem that when Ce is
used for at least part of the rare earth element and part of Co is replaced with Fe,
1-5 phase and 1-2 phase become an unstable phase and a stable phase, respectively,
and the rare earth magnet can hardly contain 1-5 phase. The present inventors have
also uncovered a problem that even when C and N are introduced as interstitial atoms
into the magnetic phase so as to stabilize 1-5 phase, the 1-5 phase cannot be sufficiently
stabilized and 1-5 phase is decomposed at high temperatures.
[0013] The present disclosure has been made to solve the problems above, and an object thereof
is to provide a rare earth magnet in which 1-5 phase is stabilized even when Ce is
used for at least part of the rare earth element and part of Co is replaced with Fe,
and a production method thereof.
[SOLUTION TO PROBLEM]
[0014] As a result of many intensive studies to attain the object above, the present inventors
have accomplished the rare earth magnet of the present disclosure and the production
method thereof. The gist thereof is as follows.
- <1> A rare earth magnet having a composition represented by the formula: (CexLa(1-x-w)R'w)v(CoyFe(1-y))(100-v-z)Mz, wherein R' is one or more rare earth elements other than Ce and La,
M represents one or more members selected from the group consisting of a transition
metal element other than Co and Fe, Ga, Al, Zn, and In, and an unavoidable impurity
element,




and

and satisfying, in the formula, the relationship of y≥-3x+1.7.
- <2> The rare earth magnet according to item <1>, further satisfying, in the formula,
the relationship of y≤-1.25x+1.25.
- <3> The rare earth magnet according to item <1> or <2>, wherein x satisfies 0.3≤x≤0.9.
- <4> The rare earth magnet according to item <1> or <2>, wherein x satisfies 0.6≤x≤0.9.
- <5> The rare earth magnet according to any one of items <1> to <4>, wherein y satisfies
0.1≤y≤0.9.
- <6> The rare earth magnet according to any one of items <1> to <4>, wherein y satisfies
0.1≤y≤0.7.
- <7> The rare earth magnet according to any one of items <1> to <4>, wherein y satisfies
0.3≤y≤0.9.
- <8> The rare earth magnet according to any one of items <1> to <4>, wherein y satisfies
0.3≤y≤0.7.
- <9> A method for producing a rare earth magnet, comprising:
preparing a molten metal having a composition represented by the formula: (CexLa(1-x-w)R'w)v(CoyFe(1-y))(100-v-z)Mz, wherein R' is one or more rare earth elements other than Ce and La,
M represents one or more members selected from the group consisting of a transition
metal element other than Co and Fe, Ga, Al, Zn, and In, and an unavoidable impurity
element,




and

and satisfying, in the formula, the relationship of y≥-3x+1.7, and
quenching the molten metal at a rate of 1×102 to 1×107 K/sec to obtain a ribbon.
- <10> The method according to item <9>, wherein in the formula, the relationship of
y≤-1.25x+1.25 is further satisfied.
- <11> The method according to item <9> or <10>, wherein x satisfies 0.3≤x≤0.9.
- <12> The method according to item <9> or <10>, wherein x satisfies 0.6≤x≤0.9.
- <13> The method according to any one of items <9> to <12>, wherein y satisfies 0.1≤y≤0.9.
- <14> The method according to any one of items <9> to <12>, wherein y satisfies 0.1≤y≤0.7.
- <15> The method according to any one of items <9> to <12>, wherein y satisfies 0.3≤y≤0.9.
- <16> The method according to any one of items <9> to <12>, wherein y satisfies 0.3≤y≤0.7.
[ADVANTAGEOUS EFFECTS OF INVENTION]
[0015] According to the present disclosure, a rare earth magnet where Ce and La are caused
to be present together in a rare earth magnet having a binary system of a rare earth
element and a transition metal element and the 1-5 phase is thereby stabilized even
when part of Co is replaced with Fe, and a production method thereof, can be provided.
[BRIEF DESCRIPTION OF DRAWINGS]
[0016]
[Fig. 1] Fig 1 is a diagram illustrating the results of Table 1 together in a formation
energy map.
[Fig. 2] Fig. 2 is a diagram illustrating the results of Table 1 together in a total
magnetic moment map.
[Fig. 3] Fig. 3 is a schematic diagram of an apparatus used for a strip casting method.
[Fig. 4] Fig. 4 is a diagram illustrating the XRD analysis results regarding samples
of Examples 1 to 5.
[Fig. 5] Fig. 5 is a diagram illustrating the XRD analysis results regarding samples
of Comparative Examples 1 to 4.
[Fig. 6] Fig. 6 is a diagram illustrating the results of calculating formation energy
of various magnetic phases.
[Fig. 7] Fig. 7 is a diagram illustrating the XRD analysis results regarding samples
of Examples 6 to 9.
[DESCRIPTION OF EMBODIMENTS]
[0017] The embodiments of the rare earth magnet of the present disclosure and the production
method thereof are described in detail below. However, the embodiments described below
should not be construed to limit the rare earth magnet of the present disclosure and
the production method thereof.
[0018] In a rare earth magnet with a binary system of a rare earth element and a transition
metal element, when the transition metal element is Co, 1-5 phase is stabilized. When
the rare earth element of 1-5 phase is a rare earth element other than a light rare
earth element, such as Sm, Nd, Pr, Dy and Tb, the 1-5 phase exhibits good saturation
magnetization.
[0019] Sm, Nd, Pr, Dy, Tb, etc. are high in rarity, compared with a light rare earth element
such as Ce, and therefore, Sm, Nd, Pr, Dy, Tb, etc. is replaced with Ce (hereinafter,
sometimes referred to as "Ce substitution"). The saturation magnetization of 1-5 phase
is reduced by Ce substitution. In order to compensate for the reduction of saturation
magnetization, Co is replaced with Fe (hereinafter, sometimes referred to as "Fe substitution").
Fe substitution enhances saturation magnetization but lets 1-5 phase be an unstable
phase and 1-2 phase be a stable phase, and the content of 1-5 phase in the rare earth
magnet decreases. Compared with 1-5 phase, the 1-2 phase is poor in both saturation
magnetization and anisotropy field.
[0020] For this reason, when Ce is used as the rare earth element, it has been conventionally
difficult to obtain a rare earth magnet containing 1-5 phase.
[0021] The present inventors have found that in the case where part of Co is replaced with
Fe in a rare earth magnet, when Ce and La are caused to be present together, CeFe
2 phase can be rendered unstable and (Ce, La)(Co, Fe)
5 phase can be rendered stable. The present inventors have also found that the ratio
(molar ratio) of Ce and La and the ratio (molar ratio) of Co and Fe, at which 1-5
phase is stabilized, can be estimated from the magnetic phase formation energy (Formation
Energy). Incidentally, (Ce, La)(Co, Fe)
5 phase indicates a phase where in the CeCo
5 phase, part of Ce is replaced with La and part of Co is replaced with Fe.
[0022] In the present description, the "1-5 phase" indicates a phase where when the magnetic
phase is represented, for example, by (Ce, La)(Co, Fe)
t phase, t is from 4 to 6 in the entire magnetic phase. Here, t being 4 to 6 means
that incomplete 1-5 phase may be contained in part of the magnetic phase. For this
reason, t is preferably from 4.5 to 5.5. Accordingly, "a magnetic phase represented
by (Ce, La)(Co, Fe)
t (wherein t is from 4 to 6, preferably from 4.5 to 5.5)" and "a magnetic phase containing
(Ce, La)(Co, Fe)
5 phase" have the same meaning.
[0023] The rare earth magnet of the present disclosure, which has been accomplished based
on the findings, etc. described hereinbefore, and the production method thereof are
described below.
<<Rare Earth Magnet>>
[0024] The rare earth magnet of the present disclosure has a composition represented by
the formula: (Ce
xLa
(1-x-w)R'
w)
v(Co
yFe
(1-y))
(100-v-z)M
z. This formula represents the entire composition of the rare earth magnet of the present
disclosure.
[0025] In the formula above, Ce stands for cerium, La stands for lanthanum, R' represents
one or more rare earth elements other than Ce and La, Co stands for cobalt, and Fe
stands for iron. M represents one or more members selected from the group consisting
of a transition metal element other than Co and Fe, Ga, Al, Zn, and In, and an unavoidable
impurity element. Ga stands for gallium, Al stands for aluminum, Zn stands for zinc,
and In stands for indium. The transition metal element is an element between Group
3 element and Group 11 element in the periodic table.
[0026] x and w are content ratios (molar ratio) of Ce and R', respectively, assuming the
entire rare earth site represented by Ce
xLa
(1-x-w)R'
w is 1. In the rare earth site, La is the remainder after removing Ce and R'.
[0027] y is the content ratio (molar ratio) of Co, assuming the entire iron group site represented
by Co
yFe
(1-y) is 1. In the iron group site, Fe is the remainder after removing Co.
[0028] v and z are contents (at%) of rare earth site and M, respectively, assuming the rare
earth magnet of the present disclosure as a whole is 100 at%. In the formula above,
the content (at%) of the iron group site is 100-v-z, and therefore in the rare earth
magnet as a whole, the iron group site is the remainder after removing rare earth
site and M.
[0029] The constituent elements of the rare earth magnet represented by the formula above
are described below.
<Ce>
[0030] Ce is a rare earth element and is an element essential for the rare earth magnet
of the present disclosure, because it develops properties as a permanent magnet. Ce
is a light rare earth element and is therefore low in rarity, compared with a medium
rare earth element and a heavy rare earth element. In conventional rare earth magnets,
when a light rare earth element such as Ce is used alone, it has been difficult to
contain 1-5 phase in the rare earth magnet. However, in the rare earth magnet of the
present disclosure, 1-5 phase is stabilized by causing Ce and La to be present together,
and 1-5 phase can thereby contain in the rare earth magnet.
[0031] In the present description, the rare earth element includes 17 elements of Sc, Y,
La, Ce, Pr, Nd, Pm, Sm, Eu, Gd, Tb, Dy, Ho, Er, Tm, Yb, and Lu. Of these, Sc, Y, La,
and Ce are a light rare earth element, Pr, Nd, Pm, Sm, Eu, and Gd are a medium rare
earth element, and Tb, Dy, Ho, Er, Tm, Yb, and Lu are a heavy rare earth element.
Incidentally, in general, the rarity of the heavy rare earth element is high, and
the rarity of the light rare earth element is low. The rarity of the medium rare earth
element is between the heavy rare earth element and the light rare earth element.
<La>
[0032] In the rare earth magnet, La is present together with Ce, and this makes CeFe
2 phase unstable and (Ce, La)(Co, Fe)
5 phase stable. Consequently, in the rare earth magnet, the content of CeFe
2 phase decreases, and the content of (Ce, La)(Co, Fe)
5 phase increases. Saturation magnetization and anisotropy field are higher in 1-5
phase than in 1-2 phase. Furthermore, in 1-5 phase, when the kind of the rare earth
element is the same, as the content of Fe is larger, the saturation magnetization
is higher. Based on these facts, the saturation magnetization reduced by Ce substitution
can be compensated for by increasing the content of (Ce, La)(Co, Fe)
5 phase.
<R'>
[0033] R' is one or more rare earth elements other than Ce and La. The rare earth magnet
of the present disclosure is obtained by causing Ce and La to be present together.
It is difficult for raw materials of Ce and La not to contain the rare earth element
R' other than Ce and La at all.
[0034] However, when the value of w in the rare earth site represented by Ce
xLa
(1-x-w)R'
w is from 0 to 0.1, the properties of the rare earth magnet of the present disclosure
can be regarded as substantially the same as those when w is 0.
[0035] Excessively increasing the purity of raw materials of Ce and La entails a rise in
the production cost, and therefore the value of w may be 0.01 or more, 0.02 or more,
0.03 or more, 0.04 or more, or 0.05 or more. On the other hand, the value of w may
be low as long as the purity of raw materials of Ce and La is not excessively increased,
and the value of w may be 0.09 or less, 0.08 or less, 0.07 or less, or 0.06 or less.
<Rare Earth Site>
[0036] The total content of Ce, La, and R' is indicated by the content v (at%) of the rare
earth site represented by Ce
xLa
(1-x-w)R'
w.
[0037] The rare earth magnet of the present disclosure has a binary system of a rare earth
element and a transition metal element. Known magnetic phases having such a binary
system include 1-2 phase, 1-5 phase, 1-12 phase, 2-7 phase, 2-17 phase, etc. The order
of these magnetic phases when arranged in descending order of rare earth element content
(in descending order of rare earth concentration) is 1-2 phase, 2-7 phase, 1-5 phase,
2-17 phase, and 1-12 phase.
[0038] In the rare earth magnet of the present disclosure, the content v (at%) of the rare
earth site is determined so as to contain 1-5 phase.
[0039] When the value of v is 7.1 at% or more, a magnetic phase smaller in the rare earth
element content than 1-5 phase, that is, 2-17 phase and 1-12 phase, etc., is less
likely to be formed, as a result, 1-5 phase is readily stabilized. From the viewpoint
of making formation of a magnetic phase smaller in the rare earth element content
than 1-5 phase difficult, the value of v is preferably 9.0 at% or more, more preferably
12.0 at% or more, still more preferably 14.0 at% or more, yet still more preferably
16.0 at% or more, even yet still more preferably 17.0 at% or more. With the value
of v in such a range, the content of the iron group site can be reduced. As a result,
α-Co phase, α-Fe phase, and α-(Co, Fe) phase are less likely to be formed as well.
Incidentally, α-(Co, Fe) phase indicates a phase where part of Co of α-Co phase is
replaced with Fe.
[0040] On the other hand, when the value of v is 20.9 at% or less, a magnetic phase larger
in the rare earth element content than 1-5 phase, that is, 1-2 phase and 2-7 phase,
etc., is less likely to be formed, as a result, 1-5 phase is readily stabilized. From
the viewpoint of making formation of a magnetic phase larger in the rare earth element
content than 1-5 phase difficult, the value of v is preferably 20.0 at% or less, more
preferably 19.0 at% or less, still more preferably 18.0 at% or less.
<Co>
[0041] As described above, the rare earth magnet of the present disclosure has a binary
system of a rare earth element and a transition metal element. As the transition metal
element, the magnet contains Co together with the below-described Fe. The rare earth
element and the transition metal element can form an intermetallic compound phase
(1-5 phase) at a molar ratio of 1:5. In the case of employing Co as the transition
metal element, in order to stabilize the 1-5 phase, Co is essential in the rare earth
magnet of the present disclosure. When Co is essential, it is easy for the rare earth
magnet to contain 1-5 phase. In addition, Co can also enhance the Curie point of the
rare earth magnet.
[0042] However, as the transition metal element contained in the rare earth magnet of the
present disclosure, Fe is essential, in addition to Co. The reason therefor is described
below.
<Fe>
[0043] As described above, 1-5 phase is higher in the saturation magnetization and anisotropy
field than 1-2 phase. Furthermore, in 1-5 phase, when the kind of the rare earth element
R is the same, RFe
5 phase is higher in the saturation magnetization than RCo
5 phase. The rare earth magnet of the present disclosure contains both Ce and La as
the rare earth element, and therefore even when part of Co of the RCo
5 phase is replaced with Fe, 1-2 phase is not stabilized but 1-5 phase remains stable.
In this way, the content of 1-5 phase having high saturation magnetization and high
anisotropy field can be increased in the rare earth magnet.
<Iron Group Site>
[0044] The total content of Co and Fe described hereinbefore is indicated by the content
of the iron group site represented by Co
yFe
(1-y). Since the iron group site is the remainder after removing rare earth site and M,
when denoting v at% as the content of rare earth site and z at% as the content of
M, the content of the iron group site is represented by (100-v-z) at%.
[0045] In the rare earth magnet of the present disclosure, binary elements of a rare earth
element and a transition metal element are the main component, and therefore M is
a subcomponent contained in the range not compromising the effects of the rare earth
magnet of the present disclosure. M is described later.
[0046] The iron group site is the remainder after removing rare earth site and M and since
M is a subcomponent, the content of the iron group site is controlled substantially
by the content v of the rare earth site. The lower limit of the content v of the rare
earth site is determined as described above, and α-Co phase, α-Fe phase, and α-(Co,
Fe) phase are thereby less likely to be formed, as a result, the stability of 1-5
phase is not hindered. On the other hand, when the upper limit of the content v of
the rare earth site is determined as described above, the transition metal element
(Co and Fe) for forming 1-5 phase does not run short easily, as a result, the stability
of 1-5 phase is not hindered.
<M>
[0047] M represents one or more members selected from the group consisting of a transition
metal element other than Co and Fe, Ga, Al, Zn, and In, and an unavoidable impurity
element.
[0048] Among M, Ga, Al, Zn, and In and transition metal elements other than Co and Fe are
elements that may be contained within the range not compromising the effects of the
present invention. In addition to these elements, M may contain an unavoidable impurity
element. The unavoidable impurity element indicates an impurity element that is unavoidably
contained or causes a significant rise in the production cost for avoiding its inclusion,
such as impurity element contained in raw materials of the rare earth magnet or impurity
element mixed in the production step.
[0049] M other than Mn (manganese), Ti (titanium) and Zr (zirconium) (excluding an unavoidable
impurity element) is present as a non-magnetic phase at an interface of the crystal
grain of 1-5 phase and enhances the coercivity of the rare earth magnet by magnetically
separating the crystal grain of 1-5 phase.
[0050] Cu among the transition metal elements and Ga, Al, Zn, and In can reduce the melting
point of a crystal grain boundary of the magnetic phase. Consequently, the crystal
grain boundary readily turns into a liquid phase during temperature rise, and therefore
the sintering (including liquid-phase sintering) temperature can be lowered.
[0051] Mn and Ti can more stabilize 1-5 phase by replacing part of Fe in 1-5 phase.
[0052] Zr can more stabilize 1-5 phase by replacing part of rare earth element in 1-5 phase.
[0053] When the value of the content z of M (including an unavoidable impurity element)
is 8.0 at% or less, the contents of rare earth site and iron group site are excessively
decreased, and therefore when the value of z is 8.0 at% or less, the effects of the
rare earth magnet of the present disclosure are not compromised. From this viewpoint,
the value of z may be 7.0 at% or less, 5.0 at% or less, 3.0 at% or less, 1.0 at% or
less, or 0.5 at% or less.
[0054] On the other hand, although the value of z may be 0 at%, it is difficult not to contain
an unavoidable impurity element at all, or a significant rise in the production cost
is caused. For this reason, the value of z may be 0.1at% or more, 0.2 at% or more,
or 0.4 at% or more.
<Relationship of x and y>
[0055] As described above, the entire composition of the rare earth magnet of the present
disclosure is represented by the formula: (Ce
xLa
(1-x-w)R'
w)
v(Co
yFe
(1-y))
(100-v-z)M
z. In addition, as described hereinbefore, in the rare earth magnet of the present
disclosure, part of Co is replaced with Fe, nevertheless, 1-5 phase is stabilized,
because part of Ce is replaced with La.
[0056] The stability of 1-5 phase is achieved by i) determining the value of v in the range
where 1-5 phase can be formed, and ii) setting a predetermined relationship between
x and y such that 1-5 phase is stabilized. Incidentally, the values of w and z are
too small to provide a substantial effect on the predetermined relationship between
x and y.
[0057] The relationship of x and y when 1-5 phase is stabilized can be determined by creating
a Ce-La-Fe-Co formation energy (Formation Energy) map. The formation energy map can
be created by calculating respective formation energies according to first-principle
calculation when changing x and y of (Ce
xLa
(1-x))(Co
yFe
(1-y))
5 phase, and applying regular solution approximation to all formation energies calculated.
[0058] As the method for first-principal calculation, a package (AkaiKKR) adopting Coherent
Potential Approximation (CPA) of the Korringa-Kohn-Rostoker (KKR) method is used.
More specifically, respective formation energies are calculated with respect to a
total of 121 points when each of x and y of (Ce
xLa
(1-x))(Co
yFe
(1-y))
5 phase is increased in steps of 10%. Then, with respect to the calculation results
of these 121 points, a formation energy map is created using regular solution approximation
formula. Incidentally, the regular solution approximation formula is as follows.
ΔE
RE5(x,y)=E
RE5(x,y)-{xyE
CeCo5+(1-x)yE
LaCe5+(1-x)(1-y)E
LaFe5+x(1-y)E
CeFe5} wherein ΔE
RE5(x,y) is change in formation energy when being x and y,
E
RE5(x,y) is formation energy when being x and y,
E
CeCo5 is formation energy of CeCo
5,
E
LaCe5 is formation energy of LaCe
5,
E
LaFe5 is formation energy LaFe
5, and
E
CeFe5 is formation energy CeFe
5.
[0059] In the thus-created formation energy map, 1-5 phase is stabilized in a small formation
energy region. The boundary between the region where 1-5 phase is stabilized and the
region where 1-5 phase becomes unstable produces a relationship that as x increases,
y decreases, and the boundary is represented by y=-3x+1.7. In addition, the region
where 1-5 phase is stabilized is a region where y is larger than in the boundary.
From these facts, the region where 1-5 phase is stabilized is a region represented
by y≥-3x+1.7.
[0060] In the region represented by y>-3x+1.7, as both x and y are further larger, the formation
energy is reduced. On the other hand, the region represented by y≤-1.25x+1.25 is a
region where as Ce increases, 1-5 phase is stabilized. The region where 1-5 phase
is stabilized may be a region represented by y≤-x+1.00.
[0061] In the region represented by y≥-3x+1.7, since Ce and La are present together and
Co and Fe are present together, it is necessary to satisfy 0<x<1 and 0<y<1.
[0062] In the region represented by y≥-3x+1.7, since the formation energy is reduced as
both x and y are further larger, x may be 0.3 or more, 0.6 or more, or 0.7 or more,
and y may be 0.1or more, 0.2 or more, 0.3 or more. Although not bound by theory, in
particular, when y is 0.3 or more, the content of Fe decreases, making production
of CeFe
2 phase difficult, and the enhancement of saturation magnetization can be more stabilized.
On the other hand, although 1-5 phase is likely to be stabilized as the formation
energy is smaller, when the formation energy is small to a certain extent, the phase
is stabilized to a degree not causing a problem in practice. Accordingly, x may be
0.9 or less, 0.85 or less, or 0.80 or less, and y may be 0.9 or less, 0.8 or less,
or 0.7 or less.
[0063] Fig. 6 shows the results of calculating formation energy Er of various magnetic phases
by the same method. As seen from Fig. 6, the LaFe
5 phase is unstable, because the formation energy Er is positive. In addition, although
the CeFe
5 phase formation energy Er is negative, since the CeFe
2 phase formation energy is lower than the CeFe
5 phase formation energy, CeFe
2 phase is more preferentially formed than CeFe
5 phase. It is seen also from Fig. 6 that Ce and La must be present together.
[0064] Furthermore, structural parameters (Fe-Fe distance, Fe-Co distance, etc.) based on
the lattice constants of CeCo
5, LaCes, LaFe
5, and CeFe
5 are calculated by first-principle calculation. As regards the structural parameters,
when the regular solution approximation formula is used, a total magnetizing moment
(Total magnetic moment) map can be created. Then, the relationship between the formation
energy and the total magnetic moment can be studied. The formation energy is related
to stability of 1-5 phase, and the total magnetic moment is proportional to magnetization,
so that the relationship between stability of 1-5 phase and magnetization can be studied
from the formation energy map and the total magnetic moment map. Incidentally, as
the method for first-principle calculation, the results of calculation using KKR-CPA
(AkaiKKR) package are supplemented by calculation using a Vienna first-principle simulation
package (Vienna ab initio simulation package (VASP) or Full potential local orbital
minimum-base code (FPLO)).
[0065] In addition, the total magnetic moment map shows that a region in which the content
of La is not excessively small relative to the content of Ce can be used to prevent
reduction of magnetization, and this is a region represented by y≤-1.25x+1.25. Although
not bound by theory, the reason therefore is believed as follows. Ce has an atomic
valence of trivalence and tetravalence, and a lot of tetravalent Ce is present in
the rare earth magnet. On the other hand, La has an atomic valence of only trivalence.
In the case of tetravalence, 4f electrons are not localized, and magnetization is
likely to disappear, but La is trivalent and since 4f electrons are localized, the
magnetization is enhanced by La. From these facts, it is considered that in the case
of causing Ce and La to be present together, the magnetization is more enhanced by
increasing the content of La. From this viewpoint, a region represented by y≤-x+1.00
is more preferred.
<<Production Method>>
[0066] The production method of a rare earth magnet of the present disclosure includes a
molten metal preparation step and a molten metal quenching step. These steps are described
one by one below.
<Molten Metal Preparation Step>
[0067] In the production method of the present disclosure, a molten metal having the same
composition as the entire composition of the rare earth magnet is prepared. The composition
of the molten metal is the composition immediately before completion of solidification.
In the case where consumption of molten metal components occurs due to evaporation,
etc. in the process of holding and/or solidifying the molten metal, the molten metal
may be prepared by blending the raw materials by taking into account the consumption.
In order to prevent the molten metal from oxidation, etc., the molten metal is preferably
prepared in an inert gas atmosphere.
[0068] In the case where the consumption of molten metal components need not be taken into
account, a molten metal is prepared by blending raw materials to afford a composition
represented by (Ce
xLa
(1-x-w)R'
w)
v(Co
yFe
(1-y))
(100-v-z)M
z. In this formula, Ce, La, R', Co, Fe, and M are the same as the contents described
for the rare earth magnet. In addition, x, w, and y as well as v and z are the same
as the contents described for the rare earth magnet. Furthermore, in this formula,
as with the description of the rare earth magnet, the relationship of y≥-3x+1.7 is
satisfied. The relationship of y≤-1.25x+1.25 may also be satisfied.
<Molten Metal Quenching Step>
[0069] A molten metal having the composition above is quenched at a rate of 1×10
2 to 1×10
7 K/sec to obtain a ribbon. This operation provides the ribbon as the rare earth magnet
of the present disclosure. In the ribbon, 1-5 phase is present, and the content ratios
(molar ratio) x and w as well as y in 1-5 phase are substantially the same as x and
w as well as y in the molten metal. Although not bound by theory, the residual liquid
in the middle of solidification, which has not turned into such 1-5 phase, forms a
grain boundary phase and is present in the rare earth magnet. In other words, in the
rare earth magnet of the present disclosure, 1-5 phase satisfying 0<x<1, 0<y<1 and
y≥-3x+1.7, i.e., a (Ce
xLa
(1-x-w)R'
w)(Co
yFe
(1-y))
t phase (wherein 0≤w≤0.1 and 4≤t≤6, preferably 4.5≤t≤5.5), is present. In the production
method of the present disclosure, x and y are set to afford a (Ce
xLa
(1-x-w)R'
w)(Co
yFe
(1-y))
t phase (wherein 0≤w≤0.1 and 4≤t≤6, preferably 4.5≤t≤5.5). Incidentally, "a (Ce
xLa
(1-x-w)R'
w)(Co
yFe
(1-y))
t phase (wherein 0≤w≤0.1 and 4≤t≤6, preferably 4.5≤t≤5.5) satisfying 0<x<1, 0<y<1 and
y≥-3x+1.7" has the same meaning as "a magnetic phase containing a (Ce
xLa
(1-x-w)R'
w)(Co
yFe
(1-y))
5 phase (wherein 0≤w≤0.1) satisfying 0<x<1, 0<y<1 and y≥-3x+1.7".
[0070] As the quenching method, for example, the molten metal can be cooled at a predetermined
rate according a strip casting method by using a quenching apparatus 10 illustrated
in Fig. 3. In the quenching apparatus 10, raw materials are melted in a melting furnace
11 to prepare a molten metal 12 having the composition above. The molten metal 12
is supplied to a tundish 13 at a fixed supply rate. The molten metal 12 supplied to
the tundish 13 is supplied to a cooling roll 14 from an end of the tundish 13 due
to its own weight.
[0071] The tundish 13 is composed of a ceramic, etc. and can temporarily store the molten
metal 12 being continuously supplied from the melting furnace 11 at a predetermined
flow rate and rectify the flow of the molten metal 12 to the cooling roll 14. In addition,
the tundish 13 also has a function of adjusting the temperature of the molten metal
12 immediately before reaching the cooling roll 14.
[0072] The cooling roll 14 is formed of a material having high thermal conductivity, such
as copper or chromium, and the surface of the cooling roll 14 is subjected to chromium
plating, etc. so as to prevent erosion with the high-temperature molten metal. The
cooling roll 14 can be rotated in the arrow direction by a drive device (not shown)
at a predetermined rotating speed. By controlling the rotating speed, the cooling
rate of the molten metal can be controlled to a speed of 1x10
2 to 1×10
7 K/sec.
[0073] When the cooling rate of the molten metal is 1×10
2 K/sec or more, 1-5 phase is contained in the ribbon. From this viewpoint, the cooling
rate of the molten metal is more preferably 1×10
3 K/sec or more. On the other hand, when the cooling rate of the molten metal is 1×10
7 K/sec or less, despite saturation of the effect obtained by quenching, the molten
metal may not be cooled at a higher rate than necessary. The cooling rate of the molten
metal may be 1×10
6 K/sec or less, or 1×10
5 K/sec or less.
[0074] In order to obtain the above-described cooling rate, the temperature of the molten
metal when supplied from the end part of the tundish 13 to the cooling roll 14 may
be 1,300°C or more, 1,350°C or more, or 1,400°C or more and may be 1,600°C or less,
1,550°C or less, or 1,500°C or less. In addition, the peripheral velocity of the cooling
roll 14 may be 10 m/s or more, 14 m/s or more, or 18 m/s or more and may be 30 m/s
or less, 28 m/s or less, or 24 m/s or less.
[0075] The molten metal 12 having being cooled and solidified on the outer periphery of
the cooling roll 14 is peeled off as a ribbon 15 from the cooling roll 14 and collected
by a collection device. If desired, the ribbon 15 may be pulverized by means of a
cutter mill, etc. to obtain a powder. The molten metal quenching step described hereinbefore
is preferably in an inert gas atmosphere as to prevent oxidation, etc. of the molten
metal.
[0076] The ribbon 15 has a crystal grain of 1-5 phase and a crystal grain boundary and therefore,
the ribbon 15 has a function as a permanent magnet by itself. A bond magnet or sintered
(including liquid-phase sintering) magnet may also be produced using the ribbon 15
or a powder obtained by pulverizing the ribbon 15.
[EXAMPLES]
[0077] The rare earth magnet of the present disclosure and the production method thereof
are described more specifically below by referring to Examples and Comparative Examples.
However, the rare earth magnet of the present disclosure and the production method
thereof are not limited to the conditions employed in the following Examples.
<<Preparation of Sample>>
[0078] A sample of the rare earth magnet was prepared in the following manner.
[0079] A molten metal having the composition shown in Table 1 was prepared using an arc
melting method, and the molten metal at 1,450°C was supplied to the surface of a cooling
roll rotating at a peripheral velocity of 20 m/s by using a strip casting method to
prepare a ribbon. The cooling rate of the molten metal was 10
6 K/s.
<<Evaluation of Sample>>
[0080] The ribbon was coarsely pulverized to obtain a powder, and the presence or absence
of 1-5 phase was confirmed by X-ray diffraction (XRD) analysis of the powder.
[0081] In addition, the ribbon was coarsely pulverized and resin-embedded, and the magnetization
properties were measured using a vibrating sample magnetometer (VSM) with a maximum
magnetic field of 9T. The measurement was performed at normal temperature (20°C).
The saturation magnetization Ms and anisotropy field Ha were calculated according
to the law of approach to saturation.
[0082] The results are shown in Table 1. In Table 1, Reference Example 1 was quoted from
J.J. Zhang et al., JMMM, 324(2012), pp. 3272-3275. Furthermore, in Fig. 1, a diagram showing the results of Table 1 together in a formation
energy map is illustrated, and in Fig. 2, a diagram showing the results of Table 1
together in a total magnetic moment map is illustrated. The formation energy map and
the total magnetic moment map were created by the methods described above. In addition,
the XRD analysis results for the samples of Examples 1 to 5 and for the samples of
Comparative Examples 1 to 4 are shown in Fig. 4 and Fig. 5, respectively. With respect
to the analysis results of each sample of Figs. 4 and 5, the upper side displays the
XRD pattern of each sample, and the lower side displays the XRD pattern of CeCo
5 phase. Incidentally, in Figs. 4 and 5, the abscissa is 2θ, and the ordinate is X-ray
intensity. The XRD analysis results for the samples of Examples 6 to 9 are shown in
Fig. 7. With respect to the analysis results of each sample of Fig. 7, the upper side
displays the XRD pattern of each sample, and the lower side displays the XRD pattern
of CeCo
5 phase. Here, the peak positions of CeCo
5 phase and (Ce, La)(Co, Fe)
5 phase are substantially the same.
[Table 1]
[0083]
Table 1
|
Target Magnetic Phase of Region |
Charge Composition (composition of molten metal) |
Value of -3x+1.7 |
Relationship of y and -3x+1.7 |
Value of -1.25x+ 1.25 |
Relationship of y and -1.25x+1.25 |
Presence of Absence o f 1-5 Phase |
Ms (T) |
Ha (T) |
Composition Formula |
x |
y |
Ce |
La |
Co |
Fe |
Example 1 |
(Ce0.35La0.65) (Co0.65Fe0.35)5 |
0.35 |
0.65 |
6.05 |
11.25 |
53.75 |
28.94 |
0.65 |
y=-3x+1.7 |
0.81 |
y<-1.25x+1.25 |
present |
1.01 |
3.07 |
Example 2 |
(Ce0.5La0.5)-(Co0.2Fe0.8)5 |
0.50 |
0.20 |
8.64 |
8.65 |
16.54 |
66.17 |
0.20 |
v=-3x+1.7 |
0.63 |
y<-1.25x+1.25 |
present |
1.05 |
3.48 |
Example 3 |
(Ce0.5La0.5)-(Co0.5Fe0.5)5 |
0.50 |
0.50 |
8.65 |
8.65 |
41.35 |
41.35 |
0.20 |
y>-3x+1.7 |
0.63 |
y<-1.25x+1.25 |
present |
1.10 |
2.39 |
Example 4 |
Ce0.65La0.35)- Co0.35Fe0.65)5 |
0.65 |
0.35 |
11.24 |
6.06 |
28.95 |
53.76 |
-0.25 |
y>-3x+1.7 |
0.44 |
y<-1.25x+1.25 |
present |
1.11 |
2.89 |
Example 5 |
Ce0.8La0.2)-(Co0.2Fe0.8)5 |
0.80 |
0.20 |
13.83 |
3.46 |
16.54 |
66.17 |
-0.70 |
y>-3x+1.7 |
0.25 |
y<-1.25x+1.25 |
present |
0.96 |
4.36 |
Example 6 |
(Ce0.5La0.5)-(Co0.8Fe0.2)5 |
0.50 |
0.80 |
8.65 |
8.65 |
66.16 |
16.54 |
0.20 |
y>-3x+1.7 |
0.63 |
y>-1.25x+1.25 |
present |
0.97 |
9.07 |
Example 7 |
Ce0.65La0.35)- Co0.65Fe0.35)5 |
0.65 |
0.65 |
11.24 |
6.06 |
53.75 |
28.95 |
-0.25 |
y>-3x+1.7 |
0.44 |
y>-1.25x+1.25 |
present |
0.97 |
3.27 |
Example 8 |
(Ce0.8La0.2)-(Co0.8Fe0.2)5 |
0.80 |
0.80 |
13.84 |
3.46 |
66.16 |
16.54 |
-0.70 |
y>-3x+1.7 |
0.25 |
y>-1.25x+1.25 |
present |
0.91 |
7.74 |
Example 9 |
(Ce0.8La0.8)-(Co0.5Fe0.5)5 |
0.80 |
0.50 |
13.84 |
3.46 |
41.35 |
41.35 |
-0.70 |
y>-3x+1.7 |
0.25 |
y>-1.25x+1.25 |
present |
0.91 |
3.49 |
Comparative Example 1 |
(Ce0.2La0.8)-(Co0.8Fe0.2)5 |
0.20 |
0.80 |
3.46 |
13.85 |
66.16 |
16.54 |
1.10 |
y<-3x+1.7 |
1.00 |
y<-1.25x+1.25 |
none |
0.95 |
2.93 |
Comparative Example 2 |
(Ce0.2La0.8)-(Co0.5Fe0.5)5 |
0.20 |
0.50 |
3.46 |
13.84 |
41.35 |
41.35 |
1.10 |
y<-3x+1.7 |
1.00 |
y<-1.25x+1.25 |
none |
1.14 |
1.68 |
Comparative Example 3 |
(Ce0.35La0.65)-(Co0.35Fe0.65)5 |
0.35 |
0.35 |
6.05 |
11.24 |
28.95 |
53.76 |
0.65 |
y<-3x+1.7 |
0.81 |
y<-1.25x+1.25 |
none |
1.16 |
2.39 |
Comparative Example 4 |
(Ce0.2La0.8)-(Co0.2Fe0.8)5 |
0.20 |
0.20 |
3.46 |
13.84 |
16.54 |
66.17 |
1.10 |
y<-3x+1.7 |
1.00 |
y<-1.25x+1.25 |
none |
1.24 |
1.62 |
Reference Example |
Ce-Co5 (document) |
1.00 |
1.00 |
- |
- |
- |
- |
-1.30 |
y>-3x+1.7 |
0 |
y>-1.25x+1.25 |
present |
0.87 |
12.7 |
[0084] As seen from Table 1 and Figs. 4 and 5, it could be confirmed that in Examples 1
to 5, the peak of 1-5 phase is clearly recognized from the XRD analysis results. Furthermore,
as seen from Figs. 1 and 2, it could be confirmed that the formation energy map and
the total magnetic moment map each created by calculation have a correlation with
the results of Table 1. Incidentally, in Fig. 1, y=-3x+1.7 is a straight line passing
through the values of Example 1 and Example 2, and y=-x+1.00 is a straight line passing
through Example 1 and Example 3.
[0085] Moreover, as seen from Table 1 and Fig. 7, it was confirmed that in Examples 6 to
9, the peak of 1-5 phase is also clearly recognized from the XRD analysis results.
Then, it could be confirmed from Table 1 that in the region of y≤-1.25x+1.25, saturation
magnetization tends to be enhanced. In addition, it could be confirmed that when y
is 0.3 or more, the enhancement of saturation magnetization is stabilized.
[0086] Although not bound by theory, the reason why the enhancement of saturation magnetization
is stabilized in the region of y being 0.3 or more is possibly as follows. Referring
to Figs. 4 and 7, in Examples 1 to 9, a peak is recognized even at a position of 2θ
being 35°. This is considered to be attributable to the fact that in Examples 1 to
9, a phase other 1-5 phase is slightly present. It is then believed that when y is
0.3 or more, the content of Fe is small and consequently, the phase other than 1-5
phase has a low possibility of being CeFe
2.
[0087] From these results, the effects of the rare earth magnet of the present disclosure
and the production method thereof could be confirmed.
[REFERENCE SIGNS LIST]
[0088]
- 10
- Quenching apparatus
- 11
- Melting furnace
- 12
- Molten metal
- 13
- Tundish
- 14
- Cooling roll
- 15
- Ribbon