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Near-field enhanced imaging by a magnetized ferrite slab

Abstract

This letter demonstrates the near-field imaging enhancement at microwave frequencies of two-dimensional sources by a ferrite slab magnetized to saturation. It is shown that this effect is based on the nonreciprocal amplification of magnetostatic surface waves (MSSW) across the ferrite slab. The inclusion of losses in our analysis has also made it possible to prove this effect for realistic yttrium iron garnet ferrite samples. For ferrite slabs of width d, the resolution at the image plane (at a distance 2d from the source) is better than the resolution in air at a distance d of the source, which leads to an equivalent air length of the ferrite slab less than zero. Since the constitutive parameters of saturated ferrites depend on the external magnetizing field, the operation frequency of the proposed imaging devices can be tuned by varying this biasing field.

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Near-field enhanced imaging by a magnetized ferrite slab

Author: Marqués Sillero, Ricardo; Mesa Ledesma, Francisco Luis; Medina Mena, Francisco
Publisher: American Institute of Physics
Year: 2005
DOI: 10.1063/1.1852091
Source: https://idus.us.es/bitstreams/f7ae24cb-039d-420e-8287-83a36496a358/download
Nea - ield enhanced imaging by a magne ized e i e slab
R. Ma qués,a)F. Mesa, and F. Medina
Depa amen o de Elec ónica y Elec omagne ismo, Facul ad de Física, Uni e sidad de Se illa,
A . Reina Me cedes s/n, 41012 Se illa, Spain
(Recei ed 3 May 2004; accep ed 17 No embe 2004; published online 4 Janua y 2005)
This le e demons a es he nea - ield imaging enhancemen a mic owa e equencies o
wo-dimensional sou ces by a e i e slab magne ized o sa u a ion. I is shown ha his e ec is
based on he non ecip ocal ampli ica ion o magne os a ic su ace wa es (MSSW)ac oss he e i e
slab. The inclusion o losses in ou analysis has also made i possible o p o e his e ec o ealis ic
y ium i on ga ne e i e samples. Fo e i e slabs o wid h d, he esolu ion a he image plane (a
a dis ance 2d om he sou ce)is be e han he esolu ion in ai a a dis ance do he sou ce, which
leads o an equi alen ai leng h o he e i e slab less han ze o. Since he cons i u i e pa ame e s
o sa u a ed e i es depend on he ex e nal magne izing ield, he ope a ion equency o he
p oposed imaging de ices can be uned by a ying his biasing ield. © 2005 Ame ican Ins i u e o
Physics.[DOI: 10.1063/1.1852091]
The p edic ion o he pe ec lens e ec in a le -handed
slab1has ce ainly g own an inc easing in e es on he ocus-
ing p ope ies o ma e ials wi h nega i e pa ame e s. In ad-
di ion o ocusing a in e media e- ield dis ances,2i has been
shown ha imp o ed nea - ield imaging can be achie ed by
means o media wi h only nega i e pe mi i i y, such as me -
als a op ical equencies.1,3 This beha io has been ound o
be a consequence o he coupling o su ace plasmons a bo h
slab in e aces.1Spin wa es wi h a beha io simila o su -
ace plasmons in me als can be ound in e imagne ic slabs
a mic owa e equencies. This ac sugges s he possibili y
o ob aining some kind o nea - ield imaging enhancemen
by employing hese ma e ials. Ex emely low-loss e i e
slabs a e p esen ly a ailable as mic owa e ma e ials. Since
losses s ongly deg ade he image enhancemen ,4 his las
p ope y o e i es can esul in a signi ican imp o emen o
he imaging. Ano he ad an age would be he unabili y o
he equency o ope a ion, which could be achie ed by
a ying he in ensi y o he ex e nal magne izing ield.
Cubic low-loss so e i es, such as y ium i on ga ne s
(YIGs), a e commonly manu ac u ed o di e se applica ions
in mic owa e echnology. When hey a e magne ized o sa u-
a ion by an ex e nal s a ic magne ic ield H0=H0z
ˆ. i s mag-
ne ic p ope ies a e well desc ibed by he so-called Polde
enso 5
␮
=
冢
␮
−i
␬
0
i
␬␮
0
001
冣
,共1兲
wi h
␮
=1+
␻
m
␻
h
␻
h
2−
␻
2;
␬
=
␻␻
m
␻
h
2−
␻
2,共2兲
whe e
␻
h=
␥
H0and
␻
m=4
␲
␥
Ms(
␥
is he gy omagne ic a-
io, and Msis he magne iza ion o sa u a ion). Magne ic
losses can be accoun ed o by he subs i u ion
␻
h→
␻
h
+共i/2兲共⌬H/H0兲
␻
, whe e ⌬His he esonance linewid h.
Magne os a ic o nonexchange spin wa es a e well known
solu ions o he elec omagne ic wa e equa ion in magne ic
media cha ac e ized by Eq. (1). They a e called magne o-
s a ic because mos o hei ene gy is associa ed wi h he
magne ic ield. The e o e, he elec ic ield can be neglec ed
in a i s o de o app oxima ion and ⵜ⫻H⬇0. Thus,
H⯝−ⵜ
␾
m, whe e
␾
mis he magne os a ic po en ial, which
mus sa is y he magne os a ic wa e equa ion,ⵜ·
␮
·ⵜ
␾
m
=0, o
冋
␮
冉
⳵
2
⳵
x2+
⳵
2
⳵
y2
冊
+
⳵
2
⳵
z2
册
␾
m=0. 共3兲
Magne os a ic su ace wa es (MSSWs)a e hose speci ic so-
lu ions o he magne os a ic wa e Eq. (3) ha a e con ined o
he su ace o he e i e.5Fo ideal lossless e i es, hey
appea when
␮
+
␬
=−1, o equi alen ly o a equency
␻
=
␻
h+1
2
␻
m. In his case, he magne os a ic po en ial akes he
o m
␾
m=
␾
0exp共−i
␻
+iky±kx兲, decaying exponen ially a
bo h sides o he e i e in e ace [see Fig. 1(a)]. The e o e,
MSSWs a e simila o su ace plasmons in many aspec s.
Howe e , due o he aniso opy o he magne ized e i e,
hey only p opaga e a he speci ic di ec ion de ined by he
wa e ec o k=kk
ˆ, wi h k
ˆ=H
ˆ0⫻n
ˆ[see Fig. 1(a)], bu no in
he opposi e one. This beha io u ns ou o be a di ec con-
sequence o he iola ion o he Lo en z ecip oci y heo em
in magne ized e i es.5
a)Elec onic mail: [email p o ec ed]
FIG. 1. (a)Rep esen a ion o he ampli ude o a MSSW a a e i e in e ace
(solid cu e). The di ec ions o he magne izing ield H0, he p opaga ion
uni ec o k
ˆ, and he su ace no mal n
ˆa e illus a ed. (b)Rep esen a ion o
he ampli ude o a MSSW in a quasipe ec nea - ield e i e ocusing
de ice.
APPLIED PHYSICS LETTERS 86, 023505 (2005)
0003-6951/2005/86(2)/023505/3/$22.50 © 2005 Ame ican Ins i u e o Physics86, 023505-1
Le us now conside he ex ension o he solu ion o Eq.
(3)ske ched in Fig. 1(a) o a e i e slab o ini e wid h das
in Fig. 1(b). The solu ion ske ched in Fig. 1(a)isaphysical
solu ion, decaying a bo h sides o he e i e in e ace. How-
e e , he e is also a ma hema ical solu ion o Eq. (3) ha
exponen ially g ows a bo h sides o he e i e in e ace and
p opaga es along he di ec ion k
ˆ=n
ˆ⫻H
ˆ0(see Re . 5). This
la e solu ion can be imposed a he le in e ace o he slab
and combined wi h he o me one a he igh in e ace o
gi e he solu ion ske ched in Fig. 1(b). This ield dis ibu ion
shows exac ly he beha io needed o he onse o he pe -
ec lens e ec ,1and becomes physical i he app op ia e
sou ce is loca ed a x=0. In ac , he ampli ude o he
MSSWs a x=0[see Fig. 1(b)] is es o ed a x=2d o all he
wa e numbe s k. Nex , i will be conside ed a wo-
dimensional ime-ha monic magne ic ield sou ce loca ed a
x=0, a a dis ance x0⬍d om he le slab in e ace. I dand
x0a e bo h much smalle han he ee-space wa eleng h
associa ed wi h he sou ce equency, we a e in he ealm o
he magne os a ic app oach. Thus, he magne ic ield p o-
duced by he ea lie sou ce can be exp essed as he ollowing
Fou ie in eg al o magne os a ic wa es (p opaga ing a bo h
di ec ions along he yaxis and decaying owa ds he e i e
slab):
␾
m共x,y兲⬇ 1
2
␲
冕
−⬁
⬁
␾
˜
m
共
k
兲
eiky−kx−i
␻
dk,共4兲
whe e
␾
˜
m共k兲is he Fou ie ans o m o
␾
m共y兲. Following
he ea lie heo y, a e se ing up a sou ce equency equal o
he equency o he MSSWs
共
␻
=
␻
h+1
2
␻
m
兲
, he ampli ude o
all he magne os a ic wa es p opaga ing along he posi i e y
di ec ion will be es o ed a a dis ance 2d om he sou ce
[see Fig. 1(b)]. On he con a y, he magne os a ic wa es
p opaga ing along he nega i e ydi ec ion will be e lec ed
by he slab, and ha dly ep oduced a he igh -hand side o
he slab. Assuming a nea ze o ampli ude o hese la e
magne os a ic wa es a x=2d[see Fig. 1(b)], he magne o-
s a ic ield ampli ude a x=2dwill be app oxima ely gi en
by
␾
m共2d,y兲⬇
冕
0
⬁
␾
˜
m
共
k
兲
eiky−i
␻
dk共5兲
o
␾
m共2d,y兲⬇1
2
␾
m
共
0,y
兲
+i
2
␲
冕
−⬁
⬁
␾
m共0,u兲
y−udu,共6兲
whe e
␾
m共0,y兲is he magne os a ic po en ial a he sou ce
plane, and he second in eg al e m can be iden i ied as he
Hilbe ans o m o his la e quan i y.6I , o ins ance, he
magne ic ield dis ibu ion a he sou ce plane is gi en by a
del a unc ion, he co esponding magne ic ield a
x=2d— he image plane—will be a del a unc ion plus he
Hilbe ans o m o his unc ion ( he 1/y unc ion). This
example illus a es how he e i e slab beha es as a quasip-
e ec nea - ield ocusing de ice.
Up o now only ideal lossless e i es ha e been consid-
e ed in he ame o he magne os a ic app oach. Howe e ,
ac ual e i es a e lossy, which subs an ially a ec s he ocus-
ing p ope ies o he e i e slab.4Mo eo e , he magne o-
s a ic app oxima ion is s ic ly alid only in he limi d→0.
In o de o ha e a comple e pic u e o he a o emen ioned
e ec s in ac ual e i e slabs, an exac elec omagne ic analy-
sis has been also pe o med. This analysis accoun s o bo h
p opaga ing and e anescen wa es in he Fou ie expansion
o he ields [a a di e ence o (4-6)]. I also accoun s o
magne ic losses by in oducing a non anishing esonance
linewid h ⌬Hin he Polde enso (1). Assuming a gi en
dis ibu ion o he ans e se- o-xmagne ic ield,
H 共0,y兲exp共−i
␻
兲, a he sou ce plane 共x=0兲, he magne ic
ield a he image plane 共x=2d兲can be exp essed as he
ollowing spec al-domain in eg al:
H 共2d,y兲=1
2
␲
冕
−⬁
⬁
关
T
共
k;
␻
兲兴
·H
˜
共
0,k
兲
eiky−i
␻
dk,共7兲
whe e H
˜
共0,k兲is he Fou ie ans o m o H 共0,y兲, and
关T共k;
␻
兲兴 is a spec al-domain ans e ma ix. This ans e
ma ix is ob ained a e sol ing he Maxwell equa ions wi h
he app op ia e bounda y condi ions a he sou ce plane, a
he ai - e i e in e aces, and o x→⬁(Somme eld adia-
ion condi ion). Thus, assuming an exp关i共ky−
␻
兲兴 phase ac-
o common o all he ields, he ans e se- o-x ields can be
ela ed by X共x,k兲=关A共k兲兴·X共0,k兲,7,8 whe e a ay X
=共Ey,Ez,Hy,Hz兲and 关A兴is a 共4⫻4兲ma ix ha only de-
pends on he cha ac e is ics and dimensions o he e i e and
ai laye s. The combina ion o he ea lie ela ion wi h he
ee space bounda y condi ion a he image plane, leads o
he ollowing exp ession o he ans e ma ix:
关T兴=兵关Z0兴−关A11兴关A21兴−1其−1 ·兵关A12兴−关A11兴
⫻关A21兴−1关A22兴其,共8兲
wi h 关Aij兴being he 共2⫻2兲subma ices o ma ix 关A兴and
关Z0兴 he ee-space impedance ma ix. Following he a o e-
men ioned p ocedu e, he Tyy e m o he ans e dyad o a
ypical low-loss YIG slab has been compu ed, and he esul s
a e shown in Fig. 2.
The ans e ma ix in ai , a a dis ance 2d om he
sou ce plane, is also shown in Fig. 2. The ans e ma ix o
he e i e slab is nea ly uni y o posi i e alues o k. This
beha io is main ained up o a maximum alue o k, which
inc eases o hinne slabs. This esul is consis en wi h he
epo ed heo y ( he hinne he slab, he be e he magne o-
s a ic app oxima ion wo ks). I clea ly sugges s a signi ican
imp o emen o he esolu ion in he p esence o he e i e
slab. In o de o illus a e his la e poin , he image o an
imposed magne ic ield a he sou ce, Hy共0,y兲, is shown in
FIG. 2. Magni ude o he yy elemen o he ans e ma ix as a unc ion o
he no malized wa e ec o k/k0共k0=
␻
/c兲 o a e i e slab as ha shown in
Fig. 1(b), wi h x0=d/2 and cons i u i e pa ame e s
⑀
=12, 4
␲
Ms=1200 G,
and ⌬H=1 Oe. The ex e nal magne izing ield is H0=520 Oe, and he op-
e a ion equency is =3.1351 GHz. Cu es o d=0.1 and 0.3 mm a e
shown (solid lines). Fo compa ison pu poses, he alues o he ans e
unc ions in ai a a dis ance 2do he sou ce a e also shown (dashed lines)
023505-2 Ma qués, Mesa, and Medina Appl. Phys. Le . 86, 023505 (2005)
Fig. 3. The imposed magne ic ield is uni y a wo hin s ips
(ma ked in he igu e)and ze o o he wise. A signi ican en-
hancemen o he image h ough he e i e can be clea ly
seen. As usual, he image h ough he e i e has been com-
pa ed wi h he alue o he Hy ield in ai , a a dis ance 2d
om he sou ce. This compa ison shows ha he equi alen
ai leng h o he e i e is less han d. In addi ion, he image
h ough he e i e has been also compa ed wi h he image
h ough ai , a a dis ance d om he sou ce. This la e com-
pa ison is o g ea in e es , since i shows ha he equi alen
ai leng h o he e i e slab is less han ze o.
Nea - ield imaging using MSSWs in e i e slabs has
se e al ad an ages o e o he me hods. One o hem is he
educed le el o losses, which p o ides a signi ican im-
p o emen o he imaging.4In ac , i is possible o ind
comme cial YIG slabs p o iding a ios ⌬H/H0o a ew hun-
d ed hs. Ano he in e es ing ad an age o he p esen p o-
posal is unabili y. Resolu ion enhancemen in slabs made o
ma e ials wi h nega i e pa ame e s is es ic ed o a single
equency ( ha p o iding he adequa e alues o he cons i-
u i e pa ame e s). The e o e, de ices made wi h his kind o
ma e ials will be usually es ic ed o a single equency o
ope a ion. Howe e , since he cons i u i e pa ame e s o e -
i es s ongly depends on he ex e nal magne izing ield, he
equency o ope a ion o imaging e i e de ices can be
uned by a ying he magni ude o his ex e nally applied
ield. The p ice o pay o hese ad an ages is ha , owing o
he aniso opy inhe en o magne ized e i es, he a o emen-
ioned o e - esolu ion can be only achie ed in he plane pe -
pendicula o he magne izing ield [ ha shown in Fig. 1(b)].
Ano he inhe en limi a ion o ocusing de ices based on he
epo ed e ec is ha hey could only ope a e in he nea -
ield limi , wi h e i e slabs o wid h dⱗ0.01␭0, whe e ␭0is
he ee space wa eleng h.
This wo k has been suppo ed by he Spanish Minis y
o Science and Technology and FEDER unds (P ojec Nos.
TEC2004-03214 and TEC2004-04249-C02-02).
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4R. Ma qués and J. Baena, Mic owa e Op . Technol. Le . 41,290(2004).
5A. G. Gu e ich, and G. A. Melko Magne iza ion Oscilla ions and Wa es
(CRC, Boca Ra on, FL, 1996).
6S. S. Haykin, Communica ion Sys ems (Wiley, New Yo k, 1983).
7C. M. K owne, IEEE T ans. Mic owa e Theo y Tech. 32,1617(1984).
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(1995).
FIG. 3. The image o an imposed magne ic ield a he sou ce plane 共x
=0兲o Fig. 1(b)gi en by Hy=1 in he s ips and ze o o he wise (do ed
line). The alue o he Hy ield a he image plane 共x=2d兲is shown (solid
line). The images in ai a a dis ance x=d(do ed line), and a a dis ance
x=2d(do -dashed line)a e also shown. Cons i u i e pa ame e s o he e -
i e a e as in Fig. 2, wi h d=0.1 mm.
023505-3 Ma qués, Mesa, and Medina Appl. Phys. Le . 86, 023505 (2005)