The technology relates to magnon laser effect.
In the parent U.S. Pat. No. 7,430,074 “GENERATION OF TERAHERTZ WAVES” the generation of nonequilibrium magnons was disclosed. In the U.S. patent application Ser. No. 11/701,284, filed on Jan. 31, 2007 and entitled “MAGNON LASER”, the generation of nonequilibrium magnons was described by using a general laser analogy.
In the present patent application a magnon laser that utilizes a magnon gain medium (MGM) at room temperatures is disclosed.
This Summary is provided to introduce a selection of concepts that are further described below in the Detailed Description. This Summary is not intended to identify key or essential features of the claimed subject matter, nor is it intended to be used as an aid in determining the scope of the claimed subject matter.
A method of generation of nonequilibrium magnons by using a magnon laser is provided. The magnon laser utilizes a magnon gain medium (MGM) selected from the group consisting of: {a ferromagnetic semiconductor; a dilute magnetic semiconductor (DMS); a half-metallic ferromagnet (HMF); and a ferromagnetic conductor, with a gap in the density of states of the minority electrons around the Fermi energy}. The half-metallic ferromagnet (HMF) is selected from the group consisting of: {a spin-polarized Heusler alloy; a spin-polarized Colossal magnetoresistance material; CrO2, Sr2FeMoO6; and Fe3 O4}.
The accompanying drawings, which are incorporated in and form a part of this specification, illustrate embodiments of the technology and, together with the description, serve to explain the principles below:
Reference now be made in detail to the embodiments of the technology, examples of which are illustrated in the accompanying drawings. While the present technology will be described in conjunction with the various embodiments, it will be understood that they are not intended to limit the present technology to these embodiments. On the contrary, the present technology is intended to cover alternatives, modifications and equivalents, which may be included within the spirit and scope of the various embodiments as defined by the appended claims.
Furthermore, in the following detailed description, numerous specific-details are set forth in order to provide a thorough understanding of the presented embodiments. However, it will be obvious to one of ordinary skill in the art that the presented embodiments may be practiced without these specific details. In other instances, well known methods, procedures, components, and circuits have not been described in detail as not to unnecessarily obscure aspects of the presented embodiments.
Recently some dilute magnetic semiconductors (DMS), with Tc above room temperature, have been studied intensively. These are oxides doped with magnetic cations. The examples are: GaN, doping Mn-9%, Tc=940 K; AlN, doping Cr-7%, Tc>600 K; TiO2 (anatase), doping Co-7%, Tc=650 K; SnO2, doping Co-5%, Tc=650 K. These magnets can be used as a magnon gain medium (MGM) to generate nonequilibrium magnons and photons at room temperatures.
Another system that can be used as a magnon gain medium (MGM) is a system comprising a half-metallic ferromagnet (HMF). Half-metallic ferromagnets (HMF) are ferromagnetic conductors, with a gap in the density of states of the minority electrons around the Fermi energy, Ef. Thus, the electrons in these materials are supposed to be 100% spin polarized at Ef. Thermal effects and spin-orbital interactions reduce the electron polarization. However, the electron polarization is close to 100% in half-metallic ferromagnets with spin-orbital interaction smaller than the minority electron gap, and at temperatures much lower than the Curie temperature Tc.
Half-metallic ferromagnets (HMF) form a quite diverse collection of materials with very different chemical and physical properties.
Chromium dioxide, CrO2. Tc=390 K. Magnetic moment per Cr=2 μB. The polarization measured at low temperatures is close to 100%. There are some other known half-metallic ferromagnetic oxides, e.g. Sr2FeMoO6.
Heusler alloys. Most of the predicted HMF are Heusler alloys. In general, these are ternary X2YZ-compounds, X and Y are usually transition metals and Z is a main group element. The most studied of them is NiMnSb: Tc=728K, magnetic moment close to 4 μB. Experiments show that NiMnSb is a half-metallic ferromagnet at low temperatures. But there is evidence that at T≈90K a phase transition into a usual ferromagnetic state takes place, and it seems unlikely that NiMnSb is a half-metallic ferromagnet near room temperature.
There are many other Heusler alloys with half-metallic ferromagnet properties, like: (1) Co2MnSi having Tc of 1034K and magnetic moment of 5 μB; (2) Co2MnGe having Tc of 905K and magnetic moment close to 5 μB, and (3) Co2MnSn having Tc of 826K and magnetic moment of 5.4 μB; etc.
It has been shown recently (S. Wurmehl et al., PRB 72, 184434 (2005)), that the alloy with the highest magnetic moment and Tc is Co2FeSi having Tc of 1100 K (higher than for Fe), and having magnetic moment per unit cell of 6 μB. The orbital contribution to the moments is small, while the exchange gap is large, of order 2 eV. Therefore, the effect of thermal fluctuations and spin-orbit interaction on the electron polarization is negligible. One should expect, therefore, that the electrons in Co2FeSi are polarized at high temperatures, sufficiently close to Tc. Indeed, according to the experiment the magnetic moment at 300K is the same as at 5K.
Colossal magnetoresistance materials: La1-xSrxMnO3 (for intermediate values of x) is presumably a half-metallic ferromagnet having Tc close to room temperature. Photoelectron emission experiments confirm the half-metallicity of La0.7Sr0.3 MnO3, with Tc=350 K. The polarization degree at T=40K is 100±5%, the gap for the minority spins is 1.2 eV.
Note that HMF, as well as ferromagnetic semiconductors, differ from “normal” metallic ferromagnets by the absence of one-magnon scattering processes. Therefore, spin waves in HMF, as well as in magnetic insulators, are well defined in the entire Brillouin zone. This was confirmed by neutron scattering experiments performed on some Heusler alloys. For references, please see: (1) Y. Noda and Y. Ishikawa (J. Phys. Soc. Japan v. 40, 690, 699 (1976)) have investigated the following Heusler alloys: Pd2MnSn and Ni2MnSn. (2) K. Tajima et al. (J. Phys. Soc. Jap. v. 43, 483 (1977)), have investigated Heusler alloy Cu2MnAl.
Hence, the magnon laser effect (disclosed in the parent U.S. Pat. No. 7,430,074 “GENERATION OF TERAHERTZ WAVES”) can be observed (in at least some of the referenced above half-metals) at room temperatures.
However, in half-metals the spin-up electron with energy larger than the exchange gap will interact with the spin-up electrons with energy smaller than the gap. Since the number of the spin-up electrons is large (as compared to the number of spin-up electrons in ferromagnetic semiconductors) this interaction should lead to the fast thermalization of high-energy electrons, which will prevent the reverse process of absorption of magnons by electrons with spin-up, which is crucial for existence of the magnon laser.
In other words, the electron bath in half-metallic ferromagnets could play the same role as the optical phonons in ferromagnetic semiconductors. However, in half-metallic ferromagnetic oxides the interaction of the electrons with spin-up with optical phonons could also play an important role.
The following disclosure is focused on magnon laser at room temperatures that can be observed in half-metallic ferromagnets, in which only the states in the lower subband are occupied in equilibrium, i.e. the electrons are fully polarized, as shown in
A nonequilibrium electron 20 put in the upper subband with spin down rapidly emits a magnon 18, with a large wave vector q≈−1 (2 mΔ)1/2, where m is the electron effective mass. It follows from the energy and momentum conservation laws that if the energy of this electron, εp, measured from the bottom of the spin down subband is much smaller than Δ, the wave vector of the emitted magnon, q lies in the interval q1≦q≦q2, where q1,2=−1 (p0±p), p0=(2mΔ)1/2, p=(2mεp)1/257 p0. The frequency of these magnons may be in the Terahertz region.
The ratio of the magnon generation rate, Γe({right arrow over (q)}), to the rate of Γm({right arrow over (q)}), their relaxation (in collisions with equilibrium magnons) is a function of the wave vector {right arrow over (q)}. Therefore the nonequilibrium magnon distribution function, N({right arrow over (q)}) has a maximum at some wave vector {right arrow over (q)}={right arrow over (q)}. N({right arrow over (q)}) increases with the increase of the electron pumping, and because of the simulated emission of magnons, the function N({right arrow over (q)}) grows most rapidly at {right arrow over (q)} close to {right arrow over (q)}*.
When the pump reaches some critical value, N({right arrow over (q)}*) starts to increase very fast with the increase of the electron pumping. At some conditions the generation of magnons with {right arrow over (q)}={right arrow over (q)}* becomes avalanche-like, and the magnon system becomes unstable. For more details, please see U.S. Pat. No. 7,430,074 “GENERATION OF TERAHERTZ WAVES”, and equations below.
Basic Equations for Magnon Generation.
The system of equations which govern the behavior of the electron, f↓({right arrow over (p)}), and magnon, N({right arrow over (q)}) distribution functions were obtained in the following paper: I. Ya. Korenblit and B. G. Tankhilevich, Sov. Phys.-JETP, 46, 1167 (1977). They read
[1+N({right arrow over (q)})]Γe({right arrow over (q)})]−[N({right arrow over (q)})−N(0)({right arrow over (q)})]Γm({right arrow over (q)})=0
f↓({right arrow over (p)})γem({right arrow over (p)})=g(εp). (Eqs. 1)
Here Γe({right arrow over (q)}) is the rate of relaxation of magnons in collisions with electrons
Γe({right arrow over (q)})=4π−1I2Sv0∫d3p(2π)−3δ(γ↑({right arrow over (p)}−{right arrow over (q)})|ε{right arrow over (p)}↓−ω{right arrow over (q)}−ε{right arrow over (p)}−{right arrow over (q)},↑)f↓({right arrow over (p)}), (Eq. 2)
where v0 is the unit cell volume.
εem is the electron-magnon relaxation rate:
γem({right arrow over (p)})=4π−1I2Sv0∫d3q(2π)−3δ(γ↑({right arrow over (p)}−{right arrow over (q)})|ε{right arrow over (p)}↓−ω{right arrow over (q)}−ε{right arrow over (p)}−{right arrow over (q)},↑)(1+N({right arrow over (q)})), (Eq. 3)
The smeared δ-function, δ(γ|ε), takes into account the finite lifetime of the electrons in the final state, caused by the interaction with electrons with spin-up (or by the interaction with optical phonons). In the case of electron thermalisation due to interaction with optical phonons
The rate ↓↑(p,εp) is the known electron damping rate due to the emission of longitudinal optical phonons (22 of
γ↑(εp)=(π/2)αΩ(≠/Δ)1/2 ln(4Δ/Ω)Δ (Eq. 5)
Here Ω is the energy of an optical phonon, and α is the strength of the electron-phonon interaction.
The function g(ε) is the generation function of electrons, with spin down. We shall treat it as a δ-function
g(εp)=g0εδ(ε−εp). (Eq. 6)
We suppose in what follows that the energy ε is small, ε57 Δ.
The second term in the l.h.s. in the first of Eqs. (1) describes the relaxation of nonequilibrium magnons in collisions with equilibrium ones, under the assumption that N({right arrow over (q)}), is close to its equilibrium value,
N(0)({right arrow over (q)})=[e(ω
Γm({right arrow over (q)}) is the magnon-magnon relaxation rate. From Eqs. (1) we obtain the following integral equation for N({right arrow over (q)}),
N({right arrow over (q)})=(N0({right arrow over (q)})+Γe({right arrow over (q)})/Γm({right arrow over (q)}))(1−Γe({right arrow over (q)})/Γm({right arrow over (q)}))−1, (Eq. 8)
where
Γe({right arrow over (q)})=g0ε∫d3pδ(γ↑({right arrow over (p)}−{right arrow over (q)})|ε{right arrow over (p)}↓−ω{right arrow over (q)}−ε{right arrow over (p)}−{right arrow over (q)},↑)δ(ε−εp)Z−1({right arrow over (p)}), (Eq. 9)
and
Z({right arrow over (p)})=∫d3pδ(γ↑({right arrow over (p)}−{right arrow over (q)})|ε{right arrow over (p)}↓−ω{right arrow over (q)}−ε{right arrow over (p)}−{right arrow over (q)},↑)(1+N({right arrow over (q)})). (Eq. 10)
Eq. (8) is formally reminiscent of the expression for the magnon distribution function under conditions of parametric pumping. The difference is that here the rate Γe is itself a functional of N({right arrow over (q)}), since the number of the emitted magnons depends on the distribution function of the electrons with spin down, f↓, which according to Eqs. (2) and (3) is in its turn determined not only by the pump g(εp) but also by a certain average (10) over the magnon distribution function. The behavior of N({right arrow over (q)}) is therefore different from that in the case of parametric pumping.
N({right arrow over (q)}) For Strong Pumping. Isotropic Case.
Let us assume for simplicity that the magnon and electron spectra are isotropic. Then Γe(q) and Γm(q) do not depend on the direction of {right arrow over (q)}. The relaxation rate Γ(q) is usually a power function of q, and it can be written as
Γm(q)=Γm(p0)(q/p0)t. (Eq. 11)
More specifically, if Γm(q) is determined by magnon-magnon exchange scattering, then t=4 for magnons, with energy ω(q0) larger than kT, and t=3 for magnons, with energy ω(q0) smaller than kT.
The strong pumping regime sets in, when g0 exceeds a critical value Gc. If the damping of electrons is due to interaction with optical phonons (and is less than (εΔ)1/2), this critical value is given by
Gc=2gc/(t+1),
gc=(Δ/ε)3/2Γm(q0)[1+N(0)(q0)]. (Eqs. 12)
At g0>Gc the function N(q) increases exponentially with pumping
N(q)=[1+N(0)(q0)](p0/2pε(t+1))exp(g0/Gc), (Eq. 13)
if q falls into the smooth region
p0−pε≦q≦p0−pε+δq,
δq=2pεexp(−g0/Gc), (Eqs. 14)
while N(q) with wave vectors outside of the above-given range does not depend on the pump. Thus, under sufficiently strong pumping the magnon distribution function has a sharp peak at q≈p0−pε.
Let us define the number of electrons, β, pumped per second per unit cell as:
β=v0(2π)−3∫d3pg(εp). (Eq. 15)
One gets for the pumping given by Eq. (6)
β=(v0ε3/2m3/2g0/21/2π23) (Eq. 16)
and the critical pumping βc, with g0=Gc is
βc=(v0q30/(2(t+1)π2))Γm(q0)[1+N(0)(q0)]. (Eq. 17)
Since we are interested in high-frequency magnons, we suppose that their relaxation is mainly due to four-magnon exchange interaction. Using the expressions for Γm given in the following reference (V. G. Vaks, A. I. Larkin and S. A. Pikin, JETP 53 (1967)), we estimated for T/TC≈0.2, and ω(q0)>kT, N(0)(q0)1: Γm≈(108-109) sec−1.
Thus, it follows from Eq. (17) the estimate βc≈(105-107) sec−1, and we took into account that N(0)(q0) is small.
The physical meaning of the critical pumping Gc can be understood as follows. The ratio Γe/Γm of the rate of generation of the magnons to the rate of their relaxation reaches its maximum value at q=p0−pε and has its minimum at q=p0+pε, i.e. there is an excess generation on the left end of the interval in comparison with the right end. Stimulated emission causes the increase of this asymmetry. Nonlinear generation begins when the difference between the number of nonequilibrium magnons at the ends of the generation interval becomes equal to the number of equilibrium magnons, if N(0)>1. On the other hand, nonlinear generation begins when the difference between the number of nonequilibrium magnons at the ends of the generation interval becomes equal to 1, if the opposite inequality (N(0)<1) holds.
In an exemplary embodiment,
The electrons pumped from the lowest energy level 38 into the highest energy level 34 move into the lower energy electron states (the first intermediate level 36) in the spin-up subband, wherein each pumped electron emits a magnon. The electrons in the spin-up subband move from the first intermediate state 36 into the bottom of the spin-up subband (the second intermediate energy level 32) by interacting with electrons with spin-up (or by emitting optical phonons). The electrons are pumped from the lowest energy level 38 into the highest energy level 34 by using a pumping means (not shown).
In an exemplary embodiment of the present technology, a conventional laser can be used as a pumping means to pump electrons form the lowest energy level (valence band) 38 into the highest energy level 34 (spin-down subband).
In an exemplary embodiment of the present technology, the four-level magnon laser (30 of
In an exemplary embodiment,
In this embodiment of the present technology, the electrons 52 injected from an external source of electrons (not shown) into the highest energy level 54 move into the lower energy electron states in the spin-up subband 58, wherein each injected electron emits a magnon. The electrons in the spin-up subband move from the intermediate energy level 58 into the bottom of the spin-up subband 62 by emitting optical phonons.
In an exemplary embodiment of the present technology, the injection means (not shown) further comprises: an electric field applied to the ferromagnetic material. In an exemplary embodiment of the present technology, the injection means is configured to inject non-polarized electrons from an external source into the ferromagnetic material, wherein the injected spin-down electrons populate the highest energy level 54. In another embodiment of the present technology, the injection means is configured to inject polarized spin-down electrons from an external source into the highest energy level 54. The polarized spin-down electrons are polarized in the direction opposite to the direction of magnetization of the ferromagnetic material.
In an exemplary embodiment, the three-level magnon laser of the present technology (50 of
In an exemplary embodiment, the four-level magnon laser of the present technology (30 of
In an exemplary embodiment, the three-level magnon laser of the present technology (50 of
Pumping Methods.
To implement the GS magnon laser of the present technology, one could use a conventional laser pumping means, as well as an electron injection means. To implement the four-level magnon laser of the present technology (30 of
Although the subject matter has been described in a language specific to structural features and/or methodological acts, the subject matter defined in the appended claims is not necessarily limited to the specific features or acts described above. Rather, the specific features and acts described above are disclosed as exemplary forms of implementing the claims.
This is a continuation-in-part of the U.S. patent application Ser. No. 11/701,284 filed on Jan. 31, 2007 now U.S. Pat. No. 7,508,578 and entitled “MAGNON LASER”, which is a continuation-in-part of the parent U.S. patent application Ser. No. 11/481,197, filed Jul. 3, 2006 U.S. Pat. No. 7,430,074 “GENERATION OF TERAHERTZ WAVES”.
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Number | Date | Country | |
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Parent | 11701284 | Jan 2007 | US |
Child | 12290527 | US | |
Parent | 11481197 | Jul 2006 | US |
Child | 11701284 | US |