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    <title>DSpace Collection:</title>
    <link>http://localhost:8081/jspui/handle/123456789/124</link>
    <description />
    <pubDate>Mon, 19 Oct 2026 21:03:56 GMT</pubDate>
    <dc:date>2026-10-19T21:03:56Z</dc:date>
    <item>
      <title>A Monte Carlo study of two dimensional Ising magnet CrI3.</title>
      <link>http://localhost:8081/jspui/handle/123456789/21743</link>
      <description>Title: A Monte Carlo study of two dimensional Ising magnet CrI3.
Authors: Aakash
Abstract: The presence of magnetic order in a layered 2D material is one of the great discoveries.&#xD;
A few years back, the presence of magnetic order in lower dimensional materials (1D&#xD;
or 2D) was not possible according to the Mermin-Wagner theorem, but the presence&#xD;
of a finite gap in the spectrum indicates a magnetic phase transition[22]. This report&#xD;
is a study of the ferromagnetic phase transition in a monolayer of chromium tri-iodide&#xD;
(CrI3). Chapter result-II shows the ferromagnetic phase transition in a monolayer of&#xD;
CrI3.&#xD;
We have started with chapter 1, in which we have described the history, method of&#xD;
production, and experimental detection of magnetism in the monolayer of CrI3 very&#xD;
briefly. After that, in Chapter 2, we discussed the layered ”CrI3” crystal structure,&#xD;
bond length, magnetic moment, etc. In chapter 3, we have studied some of the impor&#xD;
tant magnetic models, mainly the Ising model, because we are working only on the Ising&#xD;
model, followed by the Monte Carlo simulation and algorithm discussed in chapter 4.&#xD;
After that, we applied Monte Carlo simulation to square lattice and honeycomb lattice,&#xD;
and the results are presented in Chapter 5. Chapter 6 discusses some of the magnetic&#xD;
anisotropies that are responsible for the magnetic order in two-dimensional materials,&#xD;
and the final results for the monolayer of CrI3 are presented in Chapter 7.&#xD;
In the next chapter (chapter 8), we will analyse the results in various ways, like how&#xD;
we obtained the variation of specific heat with temperature for different lattice sizes. We&#xD;
have also plotted the variation of specific heat with temperature for different values of&#xD;
anisotropic constants to observe the effect of the anisotropic constant on the results. In&#xD;
the next section, we have presented the results for the monolayer of CrCl3, CrBr3, and&#xD;
CrI3 and a comparison between them to observe the effect of non-magnetic ions on the&#xD;
results. In chapter 9, the ferromagnetic phase transition is explained in great detail. We&#xD;
obtained the best fit (using polynomial fit) for our original magnetization curve. In the&#xD;
last chapter, we have listed all the results, conclusions drawn from the results, and a&#xD;
summary of the entire work.</description>
      <pubDate>Sun, 01 May 2022 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://localhost:8081/jspui/handle/123456789/21743</guid>
      <dc:date>2022-05-01T00:00:00Z</dc:date>
    </item>
    <item>
      <title>Exploring algorithms for quantum computing of atomic nuclei</title>
      <link>http://localhost:8081/jspui/handle/123456789/21742</link>
      <description>Title: Exploring algorithms for quantum computing of atomic nuclei
Authors: Gupta, Aman
Abstract: Quantum Computation techniques have been used to solve the Deuteron&#xD;
problem namely to obtain the eigenstates and eigenvalues of the groundstate&#xD;
of Deuteron. 2 encoding schemes(JWT and GC) are discussed to convert the&#xD;
Hamiltonian into sum weighted Pauli matrices. 3 quantum algorithms(VQE,&#xD;
QPE and DPE) are explored to obtain the desired properties. Modified QPE&#xD;
was also introduced to obtain the eigenstate by performing adiabatic time&#xD;
evolution of a guess state. These are algorithms are created such that it can be&#xD;
used to any nuclear many-body physics problems.</description>
      <pubDate>Sun, 01 May 2022 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://localhost:8081/jspui/handle/123456789/21742</guid>
      <dc:date>2022-05-01T00:00:00Z</dc:date>
    </item>
    <item>
      <title>ELECTRICAL AND OPTICAL HEATING OF WAVELENGTH SELECTIVE MICRORING SWITCH</title>
      <link>http://localhost:8081/jspui/handle/123456789/21741</link>
      <description>Title: ELECTRICAL AND OPTICAL HEATING OF WAVELENGTH SELECTIVE MICRORING SWITCH
Authors: Maury, Amit Kumar
Abstract: GST (Ge2Sb2Te5) is a phase change material that has recently gained attention as&#xD;
a potential materials for photonic devices due of their fast write and read speeds,&#xD;
high scalability, reversible phase change, excellent data storage, storage capacity on&#xD;
many levels and low power consumption. Electrical and optical heating of phase&#xD;
change materials (GST) embedded silicon microring with a high visual contrast during&#xD;
the GST phase shift investigate and analyse, Also in the GST amorphous phase has&#xD;
a high thermo-optic coefficient. Extinction ratios of 18.8 dB and 25.6 dB achieved&#xD;
at through and drop ports, respectively. In electrical and optical heating, GST’s&#xD;
resonance wavelength shift of almost 0.66 nm/µm and 0.40 nm/µm per unit length&#xD;
of GST, respectively achieved . Tuning efficiency in electrical and optical tuning is&#xD;
almost 0.86 nm/mW and 1.05 nm/mW, respectively. The tuning range in electrical and&#xD;
optical configuration is almost 4.57 nm and 4.04 nm, respectively for the LGST = 7 µm.&#xD;
Finally the time domain analysis of amorphization and crystallization for 1 µm to&#xD;
7 µm length of GST presented. In optical heating 80% fall time down in amorphous to&#xD;
crystalline is 54.53 ns and time to reach at room temperature is 1421.04 ns for the 1 µm&#xD;
length of GST. For crystalline to amorphous 80% fall time down in optical heating is&#xD;
36.02 ns and time to reach at room temperature is 1006.51 ns for the 1 µm length of&#xD;
GST. The same device can also be suitably used for tunable wavelength switch and&#xD;
Wavelength Selective optical power attenuator. A maximum attenuation of around&#xD;
19 dB at wavelength around 1545 nm at through port with 1 µm length of GST with&#xD;
only 0.6 mW and 1.53 mW power consumption in electrical and optical heating cases&#xD;
achieved.</description>
      <pubDate>Fri, 01 Apr 2022 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://localhost:8081/jspui/handle/123456789/21741</guid>
      <dc:date>2022-04-01T00:00:00Z</dc:date>
    </item>
    <item>
      <title>Studies of Scintillation Mechanism and Proportionality Curve by Rate Equations</title>
      <link>http://localhost:8081/jspui/handle/123456789/21740</link>
      <description>Title: Studies of Scintillation Mechanism and Proportionality Curve by Rate Equations
Authors: Mandal, Arijit
Abstract: A high energetic electron deposits energy in scintillator materials by the creation of&#xD;
electron-hole pair order of 1020 but we get the light output Photon order of 104.There&#xD;
are subsequent linear and nonlinear interactions involve within the materials.The&#xD;
radiative recombination has a non linear relation with the created primary electron&#xD;
energy. This non- proportionality relation reduces the scintillation resolution. We use&#xD;
here a system of coupled rate equations and apply it to scintillator LaBr3:Ce, CSI and&#xD;
NaI at Room temperature.The model is solved considering the transportation path of&#xD;
the carriers as cylindrical and the results are compared of these materials and total&#xD;
light yield for those materials. The space and time distributions of carriers have been&#xD;
studied to examine the response of non-proportionality. This study will give a&#xD;
detailed theoretical insight of the scintillator mechanism which will help to discover&#xD;
and fabrication of a smart scintillator with both a high light yield, better-energy&#xD;
resolution, small non-proportionality, and fast rise and decay time.</description>
      <pubDate>Fri, 01 Apr 2022 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">http://localhost:8081/jspui/handle/123456789/21740</guid>
      <dc:date>2022-04-01T00:00:00Z</dc:date>
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