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Language: en

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Hello students, welcome to lecture 25

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of the online course on Nanophotronics, Plasmonics
and Metamaterials. Today's lecture will be on

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metamaterial perfect absorbers. So here is the
lecture outline, we will first look into what

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are these metamaterial perfect absorbers and
then look into the classifications like narrow

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band perfect absorbers and broadband perfect
absorbers. We will also take an example of

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ultra-broad band perfect absorber and then we will
see the applications of these metamaterial perfect

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absorbers or MPA in short and their application in
solar energy harvesting and as thermal emitters.

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So when we talk about metamaterials, the first
thing that comes to our mind is that these are

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basically artificially engineered structures. So
where the unit cell is designed in such a way that

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can give rise to some extraordinary properties
which are not found in natural materials

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and the first thing that comes to our mind will
be the negative index material, right? Negative

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refractive index but that is not all.
When you think about other applications

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of metamaterials, one most important application
is towards light absorbing. Now light absorbing

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by any artificial structure has always been a
matter of research because you want to maximize

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the absorption. Like why you need that? Like if
you think of a solar cell where you are harvesting

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solar energy, so you want to absorb the entire
solar radiation that is falling on the solar

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cell. You do not want anything to be reflected.
What goes back is actually a waste. So you are not

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efficient if you are not able to capture all
of the solar radiation coming towards you.

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Similarly, a photodetector or any other such
devices which are supposed to harvest light,

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you want them to first act as a perfect absorber
so that you can absorb that, okay? And then you

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can convert that absorbed energy into some other
form. So light absorption is another eye-catching

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characteristic of these artificial structures
which are metamaterials and the metamaterials

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with near perfect light absorption are known as
this metamaterial perfect absorbers MPA, okay?

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Now in order to realize perfect
absorption, reflectance is suppressed.

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And how do you do that? You do that by matching
the effective impedance of the material of the

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metamaterial to that of the incident medium.
So whenever there is no impedance mismatch,

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there is no reflection. And when light falls
on an interface, there are three phenomena

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that takes place. One is reflection, one is
absorption, the other one is transmission,

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okay? So you have to somehow in absorbers, you
want the entire light to be absorbed. So you

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are trying to cancel the reflection by using some
metamaterial absorber and also you are trying to

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get rid of the transmittance. And that you can
do by introducing another metallic plate which

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acts as a mirror or by using similar mechanism
that we have seen in the multilayer system.

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So metamaterial perfect absorbers, they do not
have any transmission, they also do not have any

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reflection. So whatever falls on them should
get absorbed. Now what do you mean by perfect

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absorption? So we typically call a perfect
absorber when it is close to 99% absorption,

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okay? And it remains highly absorptive over
a wide range of incident angle, okay? For

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both TE and TM polarizations, okay? So if you
recall our discussion, previous discussions,

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at larger angle, at gazing angle, you usually
have larger reflection. But in that case, your

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light will not be that strongly absorbed.
So at larger angle, there is a possibility

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of absorption to get reduced than 99%.
But still it should be like at least more

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than 95% or so, okay? So what do you basically
take to make this kind of absorbers? Now when I

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tell you that this material is lossy, the first
thing that comes to your mind is that okay,

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this is a lossy material, so it is not very
good for waveguiding because there is high

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loss. Also it is not a very good material for
creating a resonator cavity because it will

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have low Q because it is lossy material, so the
full width of maximum will be large. But then

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lossy materials are useful, very very useful
in case of metamaterial absorbers because

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these materials can then significantly
enhance the efficiency of absorption,

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okay? So recently metamaterial perfect
absorbers have grabbed a lot of

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attention because of their near unity absorption
capability over narrow band or broadband, okay?

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So that takes us to the classification of this
metamaterial perfect absorbers. So as you can

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see the based on the wavelength range they cater
to, you can categorize them into two buckets,

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narrow band metamaterial perfect
absorbers and then you also have

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broadband metamaterial perfect absorbers. So if
you carefully look at the narrow band structure,

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here you see figure A, you can see that these
are basically overlapping rings and column

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and there is a gap between this column and the
center of the ring that is called delta x.

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So when delta x equals 0 you get almost like 90
percent of absorption, right? In this particular

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case. When you change delta x to 200 nanometer
or so you get almost 95-99 percent of reflection,

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okay? Sorry, absorption. When you further increase
it to 270 or 350 what is happening? The resonance

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is even getting sharper, so you are getting a high
Q absorption peak and you are closing towards that

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perfect absorption mark which is very very close
to unity absorption, right? So this is typically

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what I am not going to describe immediately the
physics behind this, okay? These are kind of

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symmetry breaking high Q modes, okay? And I will
just look into the features here because this is

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the narrow band. We will see in this lecture only
how to develop a structure that can give you a

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narrow band metamaterial perfect absorber
and we will also look into this particular

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structures which are able to give you broadband
metamaterial perfect absorber. So here you can

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see that it is basically a broadband absorber.
So you can see it ranges from 3 to say 5.5 micron

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where the absorption is maintained
over say 95 or 99 percent like that.

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Now what are these three arrows showing
here is that a different different regime,

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different portion of the structure is playing
the role of absorbing the light that is falling

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onto the structure. So here is the structure
this is basically a this is the tapered shape,

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okay? You can also call it tapered tooth kind of
a structure. So a different different wavelength,

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different different part of the structure
is resonating and that is able to absorb

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the electromagnetic radiation.
Here you see a short wavelength the

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top portion of the structure is absorbing most
of the incident electric field, magnetic field,

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okay? And at longer wavelength the bottom
most part of the structure which is the

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widest portion of the structure is responsible
for the absorption. Now let us look into some of

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these techniques of how do you design narrow
band metamaterial based perfect absorbers,

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okay? So here is the schematic. So you need
metal, lossy metal to design absorbers. So

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here is a schematic of a 2D array of gold discs,
okay? So the diameter is 352 nanometer and the

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thickness is 20 nanometer and the periodicity
along both X and Y directions are 600 nanometer.

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Then there is a spacer layer below this gold discs
that is MgF2 that is magnesium fluoride and it has

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got a thickness of 30 nanometer and then you have
a gold mirror which is 200 nanometer thick.

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So this is basically that portion which
is completely cancelling out any chance

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of transmission through this structure. So 200
nanometer gold film behaves like a bulk gold

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film and it is giving you zero transmittance
and it will be able to act like a good mirror,

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okay? And this entire structure is placed on top
of a glass substrate. Now you can make narrow band

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MPAs, okay? Metamaterial perfect absorbers
for which the top metallic layer is either

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patterned or unpatterned. So here we are taking a
patterned metallic layer, okay? Now in this case

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what we are using? You are using a normally
incident light with X polarization. However,

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X and Y polarization hardly make any difference
here because the structure is symmetric

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along X and Y, right? And you have taken the
permittivity of magnesium fluoride is 1.

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9 and these are the parameters that describe the
bulk gold permittivity near the near infrared

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wavelength range. You can use Drude model with a
plasma frequency of 1.37 into 10 to the power 16

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hertz, okay? And damping constant is this one,
okay? So with that you can figure out that one,

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so these are basically simulated reflection
spectrum which is plotted when the damping

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constant is considered to be 1 times,
3 times and 5 times of the bulk gold.

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So here you see when you are basically, there is
significant difference in the reflection spectrum

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or reflection dip, okay? And you can see that
when it is 3 times when the damping constant is

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basically 3 times of that of the bulk gold you are
able to get negligible reflection, okay? So it is

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0.28 percent, okay? And this is a scale up to 1
so you can understand, so this is basically 0.

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0028. So it is almost 0 reflection, right? And as
I told you in this perfect absorber A is basically

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calculated from what is reflected and then what
is transmitted these two are taken out from 1. So

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because of this bulk gold there is 0 transmission
so if there is no reflection the entire thing

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is getting absorbed, okay? So here it shows the
reflection with 0 intensity is achieved using a

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damping constant that is equal to 3 times of that
of the bulk gold. So that actually tells us that

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what should be the ideal thickness of those discs,
okay? So if you are able to use very thin discs

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so you can actually get this high damping constant
that can give you this perfect absorption. So that

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is where the design of this metamaterial comes
into picture. At resonance a strong enhancement

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of the localized electromagnetic field takes place
between the two layers the two metallic layers.

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So there is a gold disc and then there
is a gold film and in between there is

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a thin spacer layer which is a dielectric. So
this electromagnetic energy can be efficiently

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confined in this intermediate spacer layer and
that ensures that no light is reflected back.

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So you are basically trapping the energy. So
this gives rise to profound reflectance dip in

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the spectrum with nearly 0 intensity and that in
turn give rise to nearly 100 percent absorption.

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So in fact this kind of devices work as perfect
absorber over a wide range of incident angles.

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Now to better understand the nature what is
happening in this particular perfect absorber

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we should look into the current distribution
at resonance which was simulated and this is

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the figure that shows that, okay? So here you can
see that there are basically anti-parallel current

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distribution in the gold disc and the bottom gold
layer. So here it goes like this and here it is

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like this. So you can think of a circulating
current like this and this is basically

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can be thought of as a magnetic resonance
which comes from the circulating current

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and this current basically results in a magnetic
moment which strongly interacts with the magnetic

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field of the incident light. Now at resonance
what will happen? A strong enhancement of the

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localized electromagnetic field is established
between these two layers, okay And that is the

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reason why you will be having a trap of energy in
this magnesium fluoride spacer layer and no light

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is going back. Now simulation study has also
been conducted to see the angular dispersion

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of the absorption peak because right now the peak
is very very attractive it is giving you almost

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100 percent absorption but you have done only
for a normal incidence that is theta equals 0.

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Now when you do the different angle for both the
polarization these are the plots that shows you

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with frequency and angle how the absorption peak
is changing. So this is for TE polarization and

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this one is for TM polarization. So if you look at
the TM polarization first the one on the right the

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absorption peak is seen to be nearly independent
of the incident angle. So here on the y-axis you

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are varying the incident angle so it varies from
0 to 80 degrees and here you see that more or less

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it is independent of the incident angle then that
is amazing and even at 80 degree you are able to

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at the same wavelength you are able to heat almost
80 percent of absorption sorry 96 percent of

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absorption and that is that is tremendous, okay?
That is really working well and this is because

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of the fact that the direction of the magnetic
field of the incident light remains unchanged

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with various incident angles and it can
effectively drive the circulating currents

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at all angles of incidence and that is why for
TM polarization you hardly see any difference.

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However when you look into this particular
figure on the left the contour plot here the

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magnetic field cannot drive the circulating
currents efficiently at very large angles so

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any anywhere above 50 degree or so you see
the absorption has dropped significantly,

00:17:45.000 --> 00:17:54.600
okay? So at 80 degree you actually land up having
like 50 percent of absorption so that is a lot

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of drop from the perfect absorber to that.
So this is one study that tells you how to design

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metamaterial perfect absorber and always remember
that when you change the size of the disk and the

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periodicity that would help you tune the position
of this absorption peak, okay? Right now it is

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shown at a particular wavelength and it is or it
is in frequency scale so it is close to say 188

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terahertz or so and if you change the periodicity
or the size of the disk you should be able to

00:18:38.580 --> 00:18:46.320
tune that, okay? So that is how you can design
application specific narrowband perfect absorbers.

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Now moving on to the broadband perfect absorbers
let us see how you do that. Now the name itself

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tells you that you are designing something
broadband so you should have kind of a possibility

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where you can cater to multiple peaks that
can overlap spectrally and that can give

00:19:08.880 --> 00:19:14.040
rise to this broadband nature, right? So
broadband definitely you are catering to

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a much wider wavelength range right now.
So here is a schematic of that broadband

00:19:21.960 --> 00:19:28.260
absorber but surprisingly it is more or
less similar kind of a structure but then

00:19:28.260 --> 00:19:37.260
here the material property is different you are
basically using a titanium disk, okay? On top of

00:19:38.220 --> 00:19:47.340
a gold film with a silica layer on the
top acting as a spatial layer, right? So

00:19:47.340 --> 00:19:53.100
this particular schematic shows a broadband
polarization insensitive and omnidirectional

00:19:53.100 --> 00:20:01.140
absorber working in near infrared range. So that
is the range here it has been targeted to and it

00:20:01.140 --> 00:20:07.680
is based on a simple traditional metal dielectric
metal or metal insulator metal configuration.

00:20:08.400 --> 00:20:11.820
So here what happens the
highly efficient absorption

00:20:12.720 --> 00:20:20.520
is mainly coming from the excitation of
low Q localized surface plus bond resonance

00:20:21.120 --> 00:20:27.060
which are supported by the titanium nanodisks and
you are also generating the propagating surface

00:20:27.060 --> 00:20:37.080
plus bond resonance in the interface between gold
and gold film and silica. So let us look into the

00:20:37.080 --> 00:20:43.800
spectral characteristics here. So this is the
black line shows experimental result and the

00:20:43.800 --> 00:20:49.380
dotted line over there shows the simulation
result and then they are matching very very

00:20:50.760 --> 00:20:57.720
closely and you can say this like a perfect
match between simulation and experiment.

00:20:58.320 --> 00:21:05.340
So here you can see that under normal incidence so
here we are only considering theta equals 0, okay?

00:21:05.340 --> 00:21:14.220
The measured absorption of this fabricated sample
is over 90% in the spectrum ranging from 900 to

00:21:14.220 --> 00:21:24.300
1825. So this is the range till which it is more
than 90%, okay? So this is the experimental one

00:21:24.300 --> 00:21:31.320
and when you do console multi physics numerical
simulation for the same structure you also see

00:21:31.320 --> 00:21:39.720
very very similar result and in the simulation
you are basically considering a single unit cell

00:21:39.720 --> 00:21:46.380
which has got periodic boundary conditions
on both sides to repeat it in both X and Y

00:21:46.380 --> 00:21:53.160
direction and that can give you this particular
structure, okay? So numerical simulation also

00:21:53.160 --> 00:22:00.960
shows that it is very very close and because the
structure is symmetric along X and Y so it will be

00:22:00.960 --> 00:22:10.140
independent of the polarization of the incident
light and you can get very high absorption when

00:22:10.140 --> 00:22:18.540
the incident angle is less than 40 degree.
So beyond that there will be drop in the

00:22:18.540 --> 00:22:26.280
absorption. So here are some simulation
results that shows you how it works, okay?

00:22:26.880 --> 00:22:34.740
So to reveal the physics physical mechanism in
the perfect absorber you can actually plot the

00:22:34.740 --> 00:22:40.800
electric and the magnetic fields, okay? At the
two absorption peaks so if you carefully see that

00:22:40.800 --> 00:22:46.200
there is basically one peak and then there is
another peak here, okay? So there are basically

00:22:46.200 --> 00:22:52.320
two peaks which are spectrally overlapping one is
a narrow peak and another one is a pretty broad

00:22:52.320 --> 00:23:02.580
peak. So there is a peak at 914 and another one
at 1468 nanometer, okay? And if you look into the

00:23:03.960 --> 00:23:10.860
electric field distribution these two resonances
both look like electric dipolar resonances,

00:23:10.860 --> 00:23:18.360
okay? On the nanodiscs when you are
considering the TM polarization. However,

00:23:18.360 --> 00:23:24.540
the magnetic field distribution that you see
here is pretty different in these two cases.

00:23:25.140 --> 00:23:33.000
And if you also analyze that what is the origin
of this peak then you can say that the short

00:23:33.000 --> 00:23:39.300
wavelength resonance that you are seeing at
914 nanometer is basically considered to be

00:23:39.300 --> 00:23:47.580
the propagating surface plus bond PSP, okay?
Resonance that comes between the continuous

00:23:47.580 --> 00:23:55.560
gold film and the silica spacer where the
magnetic field is not only strongly confined in

00:23:55.560 --> 00:24:03.540
the gap region between the nanodiscs but also
strongly enhanced between the nanodiscs.

00:24:04.500 --> 00:24:13.860
And the other case which is the long wavelength
mode so at you can call this as lambda 2 this

00:24:13.860 --> 00:24:19.920
one is lambda 1. So you can say the long
wavelength mode which is at lambda 2 1468

00:24:19.920 --> 00:24:26.400
nanometer this is basically a localized surface
plus bond resonance peak where the magnetic field

00:24:27.840 --> 00:24:36.420
is mainly concentrated within the gap between
the topmost nano antennas and the gold underlay,

00:24:36.420 --> 00:24:43.860
okay? And since titanium is dispersive it is very
dispersive and has a relatively large imaginary

00:24:43.860 --> 00:24:49.440
part okay if you look into the dispersion relation
you will get to know that the intrinsic absorption

00:24:49.440 --> 00:24:58.140
coefficient of titanium is very large, okay?
So you can actually understand that the quality

00:24:58.140 --> 00:25:05.220
factor of the resonance of this localized surface
plus bond resonance peak here is rather low and

00:25:05.220 --> 00:25:14.340
that gives you this broadening of the absorption
and that is how and this is the difference between

00:25:15.180 --> 00:25:22.440
that gold discs and titanium discs and why we
actually opted for titanium discs here when we

00:25:22.440 --> 00:25:29.160
are planning to make a broadband absorber,
okay? So once again we can attribute this

00:25:29.160 --> 00:25:36.420
broadband absorption to the combination effect of
propagating surface plus bond and low Q localized

00:25:36.420 --> 00:25:47.940
surface plus bond resonance. Now you can see here
some of the parametric sweep result it means like

00:25:47.940 --> 00:25:55.860
the influence of some parameters on the absorption
performance and how the absorption spectra looks

00:25:55.860 --> 00:26:03.840
like for different materials. So this one is a
simulated result where d is the disc diameter that

00:26:03.840 --> 00:26:12.420
has been changed from 380 to 400 to 420 nanometer.
The same thing is also seen experimentally and you

00:26:12.420 --> 00:26:19.200
can see how it changes so they are sensitive to
the dimensions as I mentioned so you can actually

00:26:19.200 --> 00:26:27.780
design the discs based on your requirement.
So again the periodicity is changed here and

00:26:27.780 --> 00:26:36.120
the periodicity also tells you it actually gives
you the range over which you want to have this

00:26:36.120 --> 00:26:43.140
broadband absorption. So here periodicity of
580, 600 and 620 nanometer has been studied

00:26:43.140 --> 00:26:47.640
and simulated results and experimental results
they are very very close to each other,

00:26:47.640 --> 00:26:54.660
right? And here also you can see if you take the
contribution to this absorption coming from gold

00:26:54.660 --> 00:27:02.640
and titanium you can clearly see that titanium
is contributing to the most of the absorption.

00:27:02.640 --> 00:27:09.600
So that is the case here this absorber is
mainly based on this titanium nano discs.

00:27:09.600 --> 00:27:16.140
Now we understood that how we can make narrow band
we understood how we can make broadband absorbers

00:27:16.140 --> 00:27:23.700
now we have to understood we have to understand
how we can make ultra broadband metamaterial

00:27:23.700 --> 00:27:31.380
based perfect absorbers. When I say ultra
broadband I am thinking of a window something

00:27:31.380 --> 00:27:39.480
as large as 300 to say 4500 nanometer.
So it starts from typically you know UV

00:27:39.480 --> 00:27:48.540
visible near infrared and then short and mid IR
something like that. So it is typically catering

00:27:48.540 --> 00:27:56.700
to a very very broadband and this is the kind
of structures we call them as ultra broadband

00:27:56.700 --> 00:28:01.860
absorbers. So how do you make it? You can
actually design them using 2D infinite array of

00:28:01.860 --> 00:28:07.680
hemi ellipsoid shaped metallo-dielectric
multilayer structures. So here is the top view

00:28:07.680 --> 00:28:14.220
of the structure so these and this is the side
view so you can see it is like a hemi ellipsoid

00:28:14.220 --> 00:28:20.580
so half of the ellipsoid and it is alternating
metal dielectric metal dielectric structure. So

00:28:20.580 --> 00:28:28.680
it is based on a silicon substrate but then you
have a ground metal ok it is it can be gold it

00:28:28.680 --> 00:28:35.100
or silver it can it has to be 300 nanometer so it
blocks light completely and it will reflect ok.

00:28:35.100 --> 00:28:40.740
And then you have dielectric metal dielectric
metal you have these are the simulation setup

00:28:40.740 --> 00:28:47.100
basically with PML perfectly matched layers.
So this allows you to do a simulation of this

00:28:47.100 --> 00:28:53.280
particular structure for TM polarization ok.
Here the H field is considered to be along Y

00:28:53.280 --> 00:29:01.800
axis and the wave propagation is considered to be
along Z axis ok and port 1 is the excitation port

00:29:01.800 --> 00:29:08.520
and port 2 is the other port. So if you
calculate S11 you can get the reflection

00:29:08.520 --> 00:29:13.980
characteristics and if you calculate S21 you
can find out the transmission characteristics

00:29:13.980 --> 00:29:19.980
from the S parameter matrix ok. And here is
the periodicity P that is basically the size

00:29:19.980 --> 00:29:28.980
D and the gap G between the hemi ellipsoids.
So how many layers we have considered 20 layers

00:29:28.980 --> 00:29:36.540
of metal dielectric alternate structures here
molybdenum and germanium are considered and

00:29:37.200 --> 00:29:46.320
not gold we are using tungsten as a ground metal
and this is standing over a silicon substrate ok.

00:29:46.320 --> 00:29:51.540
So a perfectly matched layer as I mentioned
has been applied here on the top and bottom

00:29:51.540 --> 00:29:56.340
of the unit cell. So this is the side view of
the unit cell this is the top view of the unit

00:29:56.340 --> 00:30:03.960
cell that you can see here. d is the diameter
of this hemi ellipsoid the base diameter that

00:30:03.960 --> 00:30:11.580
is 400 nanometer and then gap is 20 nanometer
ok. The periodicity is 420 nanometer and these

00:30:11.580 --> 00:30:16.860
are the parameters that we have used and other
parameters are mentioned in this particular

00:30:16.860 --> 00:30:25.020
figure I will not read out each of them.
And then we have then using the RF module of the

00:30:25.020 --> 00:30:33.120
console multi physics software the absorption
spectrum has been calculated for 300 to 500

00:30:33.120 --> 00:30:40.560
nanometer spectral window ok. And this allows one
to get absorption reflectance and transmittance

00:30:40.560 --> 00:30:46.680
for this structure at normal incidence. So
this is that particular structure absorption

00:30:46.680 --> 00:30:53.340
reflectance and transmittance and as you can see
here the transmittance the red one is completely

00:30:53.340 --> 00:30:59.520
flat. So there is zero transmittance across the
structure and you can also see that the absorption

00:30:59.520 --> 00:31:10.260
reflectance sorry absorption is almost 100 percent
of other than this few ringing effects that come

00:31:10.260 --> 00:31:19.200
from multiple resonance here ok. And more or
less it is a very flat wide band absorption ok

00:31:19.200 --> 00:31:26.400
and what is not absorbed is kind of reflected.
So the green curve shows you the reflection curve

00:31:26.400 --> 00:31:33.000
and this is the plot for the two polarization TE
and TM polarization for normal incidence and they

00:31:33.000 --> 00:31:38.820
are perfectly matching because the structure
is also symmetric right. So this particular

00:31:38.820 --> 00:31:46.260
structure as I mentioned it is a ultra broadband
metamaterial based perfect absorber or this kind

00:31:46.260 --> 00:31:52.320
of absorbers are also called super absorbers
because they give you almost 99 percent average

00:31:52.320 --> 00:32:01.440
absorption and that is a big thing 99 percent
average absorption between 300 to 400 nanometer

00:32:01.440 --> 00:32:07.920
spectral range at normal incidence. And this
particular spectral range it comprises as I

00:32:07.920 --> 00:32:14.760
mentioned earlier UV visible near infrared
short wave and mid wave infrared wavelength.

00:32:14.760 --> 00:32:24.780
So that is pretty wide range ok. So this kind
of metamaterial absorbers can be designed.

00:32:24.780 --> 00:32:30.240
Now let us look into the applications of
this metamaterial perfect absorbers. The

00:32:30.240 --> 00:32:36.240
first application that comes to our mind is solar
energy harvesting and when we talk about solar

00:32:36.240 --> 00:32:41.880
energy harvesting the most important thing for us
is to know that how the solar spectrum looks like

00:32:41.880 --> 00:32:51.780
ok. So you can see this is the solar spectrum or
solar spectral radiation ok versus wavelength. So

00:32:51.780 --> 00:32:59.940
it actually follows this particular pattern ok. So
you can actually have a blackbody radiation that

00:33:02.040 --> 00:33:10.620
blackbody radiation picking around 5500 I believe
ok that can match this 5500 Kelvin ok that can

00:33:10.620 --> 00:33:14.940
match this particular solar spectrum.
But then what is important here is that

00:33:14.940 --> 00:33:20.100
it tells you the range over which you are
supposed to absorb. Now if you do not absorb

00:33:20.100 --> 00:33:26.280
anything beyond say 1800 you are not losing
much you are only having a very small portion

00:33:26.280 --> 00:33:33.360
of the solar spectrum which lies beyond 1800.
So you can actually design your absorber until

00:33:33.360 --> 00:33:39.240
here ok. There are many atoms basically
in the literature to design this kind of

00:33:39.960 --> 00:33:46.860
perfect absorber. One such design has been
published in this paper that I am showing here.

00:33:46.860 --> 00:33:55.500
So this is a broadband absorber where you have a
periodic square array of silica which are coated

00:33:55.500 --> 00:34:07.140
with iron film ok and this is separated from
a bottom iron mirror by another silica film

00:34:07.140 --> 00:34:15.900
and a GST film. So this is the 3D view and this
is the 2D view of the structure. Again you can

00:34:16.800 --> 00:34:23.880
calculate what is the spectral absorptivity of
this structure. You can see that this structure

00:34:24.780 --> 00:34:33.180
can absorb very strongly from 400 to 2000
that is the entire band that we are looking

00:34:33.180 --> 00:34:39.120
for ok. Now this is the absorption that
is from this particular structure.

00:34:39.120 --> 00:34:45.720
Now if we tweak this structure a little bit or
you redesign this structure your aim would be

00:34:45.720 --> 00:34:53.580
to have a flat absorption line over this entire
window and the discussion we had previously those

00:34:53.580 --> 00:35:02.220
kind of structures can give you almost 100% of
absorption over this band. Now the question is

00:35:02.220 --> 00:35:08.040
why then we need to design this one again if
that previous structure is giving us all that

00:35:08.040 --> 00:35:12.900
we need. Now if you see the previous structure
fabrication wise that structure is very very

00:35:12.900 --> 00:35:19.800
challenging. It is a hemispherical shape with
alternating layers of metal dielectric and then

00:35:19.800 --> 00:35:28.500
you have to maintain that reducing dimension as
well. So that is a very challenging structure on

00:35:28.500 --> 00:35:33.780
in comparison to that this is much easier
structure and that can give you an average

00:35:33.780 --> 00:35:40.500
absorption of almost a 90% or so 90 to 95%.
So in some cases where you do not have the

00:35:40.500 --> 00:35:46.860
facility to fabricate those complicated structures
you can still be happy with this kind of a

00:35:46.860 --> 00:35:54.720
structure. What are the other applications?
So this one is basically an application of

00:35:54.720 --> 00:36:03.420
a broadband metamaterial perfect absorber.
Now you can also have applications of narrow

00:36:03.420 --> 00:36:09.960
band metamaterial perfect absorbers as thermal
emitters. Now what are these thermal emitters?

00:36:10.620 --> 00:36:17.940
Now if you think of a black body it is basically
an idealized body that can absorb all radiation

00:36:19.320 --> 00:36:25.500
which falls on it and it re-radiates
energy solely determined by its temperature

00:36:26.400 --> 00:36:34.620
as described by the Planck's law. Now when
you develop metamaterials okay and you are

00:36:34.620 --> 00:36:42.540
targeting an application of perfect absorber
which exhibits the ability to have near uniform

00:36:42.540 --> 00:36:48.840
or near unity absorption in a frequency range
you are basically making it like a black body.

00:36:49.500 --> 00:36:54.840
So this same material can also behave
like a thermal emitter right just like

00:36:54.840 --> 00:37:00.600
black body radiates your metamaterial can also
radiate. According to Kirchhoff's law of thermal

00:37:00.600 --> 00:37:06.660
radiation at equilibrium the emissivity
of a material equals to its absorptivity.

00:37:07.260 --> 00:37:13.440
Therefore in principle the metamaterial perfect
absorbers can radiate energy as described by their

00:37:13.440 --> 00:37:20.760
absorptivity at a given temperature. Now because
of the resonant nature of the metamaterials

00:37:20.760 --> 00:37:27.480
the perfect absorber the narrowband perfect
absorbers they yield very sharp resonances

00:37:27.480 --> 00:37:33.720
with high absorption that means they will
basically act as very high q thermal emitters

00:37:34.320 --> 00:37:41.460
and they will also have very high emissivity.
So that way you can actually make very high q

00:37:41.460 --> 00:37:47.760
high emissivity thermal emitters.
So here is one design of infrared

00:37:48.720 --> 00:37:53.640
metamaterial absorber that will also work as a
thermal emitter we will see that. So here is a

00:37:53.640 --> 00:38:00.720
structure first you start with a plus type okay
plus kind of a structure. So this is a metallic

00:38:00.720 --> 00:38:06.240
structure gold structure on a dielectric and on
the back side also you have another gold layer

00:38:06.240 --> 00:38:12.840
okay. So this is the top view of the single
band metamaterial absorber and these are the

00:38:12.840 --> 00:38:18.540
dimensions okay all are in microns here
length, width, periodicity all are given

00:38:19.140 --> 00:38:25.920
okay and this is a dual band so this is basically
a mixture of the small and the large there are

00:38:25.920 --> 00:38:32.100
two structures which resonate at two different
frequency band and that is why it is called a

00:38:32.100 --> 00:38:39.900
dual band metamaterial absorber and the dimensions
are given here all are in microns again. And these

00:38:39.900 --> 00:38:48.180
two shows the top view these two figure shows
the perspective view and in the two cases the

00:38:48.180 --> 00:38:54.600
thickness of the dielectric spacer is 0.
2 micron here for the single band metamaterial

00:38:54.600 --> 00:38:59.700
absorber and it is 0.3 micron in the
case of dual band metamaterial absorber.

00:39:00.660 --> 00:39:08.820
Now when you do the experimental absorption study
of this structure so here in the inset you can see

00:39:08.820 --> 00:39:17.700
the SEM images. So for the single band structure
you get this peak which is pretty good and also

00:39:17.700 --> 00:39:24.240
these are all experimental pictures okay for
the dual band you get these two bands which

00:39:24.240 --> 00:39:32.880
are absorbing very strongly right. So that
way you can also compare the experimental

00:39:32.880 --> 00:39:38.940
absorptivity with the emissivity and you see
that they do follow the law of Kirchhoff that

00:39:38.940 --> 00:39:46.020
we have discussed that the absorption pattern
is same as their emission spectrum right.

00:39:47.280 --> 00:39:58.920
So that way you can actually see that you can
develop a thermal emitter a high Q thermal

00:39:58.920 --> 00:40:04.680
emitter at a single band a dual band or multiple
bands depending on the design of your metamaterial

00:40:04.680 --> 00:40:14.520
absorber okay. So this one shows the absorptivity
and emissivity of a single band absorber or you

00:40:14.520 --> 00:40:22.320
can say emitter whereas this one shows a dual
band absorber or emitter okay. So that way you

00:40:22.320 --> 00:40:27.780
can actually design the materials. So what
is important here you to understand that the

00:40:27.780 --> 00:40:34.020
structures the emission spectrum spectrum is
completely dependent on the structure that you

00:40:34.020 --> 00:40:40.080
are designing okay. If you choose a different
shape, if you choose a different material,

00:40:40.080 --> 00:40:46.620
if you choose a different periodicity or a
thickness the resonance peak can be changed.

00:40:46.620 --> 00:40:53.220
If you want to play with the Q factor of
the resonance you can choose if you want

00:40:53.220 --> 00:41:01.920
to lower high Q okay means you want a sharper
resonance peak you should select materials which

00:41:01.920 --> 00:41:10.980
are less lossy and then if you want a resonance
with a broader Q okay you should actually choose

00:41:10.980 --> 00:41:16.800
materials with high loss that we have seen.
Now while choosing the material properties

00:41:16.800 --> 00:41:23.280
you got to be very careful about the dispersion.
So you have to choose the material property that

00:41:23.280 --> 00:41:29.820
is suitable for the range the frequency range
that you are considering. So usually there are

00:41:29.820 --> 00:41:36.360
websites like refractiveindex.info where you
can download and see the dispersion curves of

00:41:36.360 --> 00:41:43.800
different materials and that helps you understand
which material could be useful in designing what

00:41:43.800 --> 00:41:52.740
kind of emitters at what frequency band okay.
So with that I think we have covered the topics

00:41:52.740 --> 00:42:01.260
and that is all for this lecture we will
consider the topics of smart sorry superlens

00:42:01.260 --> 00:42:06.660
and hyperlens in the next lecture and in case
you have got any queries on this particular

00:42:06.660 --> 00:42:12.660
lecture you can drop an email to this email
address with in the subject line. Thank you.
