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  <title>DSpace Community:</title>
  <link rel="alternate" href="http://hdl.handle.net/123456789/2" />
  <subtitle />
  <id>http://hdl.handle.net/123456789/2</id>
  <updated>2023-04-07T16:38:09Z</updated>
  <dc:date>2023-04-07T16:38:09Z</dc:date>
  <entry>
    <title>Conjugated polyacetylenes in a high-intensity circularly polarized laser</title>
    <link rel="alternate" href="http://hdl.handle.net/123456789/2058" />
    <author>
      <name>Charapale, Omkar Namdev</name>
    </author>
    <id>http://hdl.handle.net/123456789/2058</id>
    <updated>2022-12-23T19:22:30Z</updated>
    <published>2022-04-01T00:00:00Z</published>
    <summary type="text">Title: Conjugated polyacetylenes in a high-intensity circularly polarized laser
Authors: Charapale, Omkar Namdev
Abstract: In last decades, light matter interaction pushed to laser induced atomic and molecular&#xD;
electron dynamics. Solving Schr Ö dinger equation with laser purtubed hamiltonian&#xD;
by using Hartree-Fock theory brings a way to observe evoultion of molecular orbitals&#xD;
and their energies with time. Here, we have performed a computation where laser&#xD;
has been induced on polyacetylens with fixed nuclear states to observe effects to&#xD;
π electron delocalization. Molecular electron density (MED) which is scalar field&#xD;
and physically observable quantity is useful to gain knoweldge of chemical anologies&#xD;
from topological point of view. The topographical analysis brings out changes in&#xD;
number and nature of critical points corresponding to reorientation of electron cloud.&#xD;
Bond saddle which gives insightment to hypothetical nature of chemical bond and&#xD;
its bond ellipticity to measure anisotropy and π character were extensively studied&#xD;
and analysed with propogation. In the presence of laser, bond critical point between&#xD;
C and H approches towards H, providing charge redistribution, decrease in size&#xD;
of basin and AIM atomic charge and so increase in electropositive charactor for H&#xD;
attractor, bond polarity of C-H bond and overall acidity of molecule. Slight shift to&#xD;
higher intensity regime affects MED bifurcating acetylenic bcp, forming more regions,&#xD;
basins and active reaction sites.</summary>
    <dc:date>2022-04-01T00:00:00Z</dc:date>
  </entry>
  <entry>
    <title>Attempts to identify folate transporters in saccharomyces cerevisiae /</title>
    <link rel="alternate" href="http://hdl.handle.net/123456789/2057" />
    <author>
      <name>Vedula, Sahithi</name>
    </author>
    <id>http://hdl.handle.net/123456789/2057</id>
    <updated>2022-12-23T19:18:51Z</updated>
    <published>2022-04-01T00:00:00Z</published>
    <summary type="text">Title: Attempts to identify folate transporters in saccharomyces cerevisiae /
Authors: Vedula, Sahithi
Abstract: Folate is an important micronutrient for all the organisms. Many prokaryotes and eukaryotes&#xD;
can synthesize folates de novo, but humans require a dietary intake of folates. Folate uptake&#xD;
in human cells is mediated by transporters on the plasma membrane namely SLC46A1 and&#xD;
SLC19A1, but there are no known homologs in yeast. Although yeast can synthesize folates,&#xD;
it can also take folates exogenously, suggesting the presence of folate transporters. Yet, folate&#xD;
transporters have not been identified in yeast. So, the study aims to identify folate&#xD;
transporters in yeast. As there were no detectable homologues of SLC19A1 and SLC46A1 in&#xD;
yeast, a strategy was designed making use of synthetic lethality of yeast fol2 mutant with&#xD;
putative transporter deletion mutants. The FOL2 gene of Saccharomyces cerevisiae encodes&#xD;
the enzyme GTP cyclohydrolase. Hence fol2Δ was to be created in a library of putative folate&#xD;
transporter deletion strains ordered from EUROSCARF. The fol2Δcassette was improved by&#xD;
increasing the length of the homologous region for better in vivo recombination in yeast.&#xD;
Yeast spotting assay was performed to examine if any of the double deletion strains exhibited&#xD;
growth defectsin suboptimal concentrations of folinic acid ranging from nil, suboptimal and&#xD;
optimal folinic acid concentrations. With fol2 deletion background, the strains with ORFs&#xD;
YER039cΔ, YER060w-aΔ, YJL163cΔ, YOR306cΔ, YOR071CΔ, YBR132CΔ, YBR220cΔ,&#xD;
YCL049cΔ, YNR062cΔ, YML038cΔ, YGL186cΔ, YDR406wΔ, YPL274wΔ, YGR260wΔ,&#xD;
YOL162wΔ, YIR028WΔ showed distinct slow growth compared to BY4741 with fol2∆.One&#xD;
possible explanation for the result is that there might be more than one folate transporter in&#xD;
yeast. Insilico analysis of the promoters of the major genes of folate biosynthesis pathway,&#xD;
namely FOL1, FOL2, FOL3, MTD1, DHFR, MET7 was performed for four Saccharomyces&#xD;
species i.e. Saccharomyces cerevisiae, Saccharomyces paradoxus, Saccharomyces mikatae,&#xD;
Saccharomyces bayanus to identify some conserved boxes. Though some conserved regions&#xD;
were identified no region was conserved across the genes highlighting that the genes are&#xD;
regulated via different modes if at all any regulation exists. Further narrowing down to FOL2&#xD;
gene promoter to check it is regulated in the presence of folinic acid. 800bp upstream of&#xD;
FOL2gene was cloned under lacZ reporter gene. Currently, I am testing it for positive clones;&#xD;
the cloning is ongoing, and assay will be performed after that.</summary>
    <dc:date>2022-04-01T00:00:00Z</dc:date>
  </entry>
  <entry>
    <title>Multi-wavelength study of magnetic cataclysmic variables using astrosat</title>
    <link rel="alternate" href="http://hdl.handle.net/123456789/2056" />
    <author>
      <name>Samantaray, Abhinna Sundar</name>
    </author>
    <id>http://hdl.handle.net/123456789/2056</id>
    <updated>2022-12-23T19:14:45Z</updated>
    <published>2022-04-01T00:00:00Z</published>
    <summary type="text">Title: Multi-wavelength study of magnetic cataclysmic variables using astrosat
Authors: Samantaray, Abhinna Sundar
Abstract: Magnetic Cataclysmic Variables (MCVs) are the semi-detached binary systems where&#xD;
the primary White Dwarf (WD) accretes matter from the Roche-lobe filled secondary main&#xD;
sequence star. MCVs can be classified into Polars and Intermediate Polars (IPs) on the basis&#xD;
of magnetic field strength of the WD. MCVs emit over broad wavebands due to the continu-&#xD;
ous interaction between the two components. These systems provide a better understanding&#xD;
of the nature of accretion in the presence of magnetic fields &amp; can be used to understand&#xD;
their evolutionary states. This thesis outlines the multi-wavelength study of three MCVs&#xD;
using AstroSat. These are AR UMa (Polar), QS Tel (Polar), and 1RXS J161935.7+54630&#xD;
(Polar/Asynchronous Polar). To accomplish our aim, we used AstroSat space observatory&#xD;
for observations in Near UV, Far UV and Soft X-rays. A detailed temporal and spectral&#xD;
analyses was performed for the three MCVs. By observing in both UV and X-ray regimes,&#xD;
we co-relate spectral energy distributions, fluxes, and spectral variations of these systems.&#xD;
AR UMa (AR Ursae Majoris) has the strongest magnetic field found in an accreting&#xD;
Polar. From timing analysis, we found that its orbital period is P Ω = 1.93 hrs, consistent&#xD;
with the literature. The mean AB magnitude was estimated to be 16.18 ± 0.20 in NUV&#xD;
and 15.95 ± 0.28 in FUV region. AR UMa was not detected in soft X-rays and was in its&#xD;
‘faint’ state during the observation period. 1RXS J161935.7+524630 (DDE 32), a newly&#xD;
discovered MCV located in the constellation of Draco. It is very first time that the Multi-&#xD;
wavelength study is performed on this system. The orbital period of this MCV was found&#xD;
to be 2.01 hrs. The source was in low accretion state with mean AB magnitudes of 19.27 ±&#xD;
1.20 and 20.31 ± 0.93 in NUV and FUV regimes respectively and was X-ray silent too.&#xD;
Lastly, we also observed QS Telescopii (QS Tel), a MCV containing 50 − 80 MG White&#xD;
Dwarf, lies in the period gap of CVs having an orbital period of P Ω = 2.32 hrs. We found&#xD;
that this system was in its low state during AstroSat observation with mean AB magnitudes&#xD;
of 17.08 ± 0.17 in NUV and 17.06 ± 0.54 in FUV filters. This was the only source observed&#xD;
in soft X-rays with black-body temperature of 0.09 keV and thermal plasma temperatures of&#xD;
0.57 &amp; 20.7 keV from post-shock region, for hydrogen column density of 4.38×10 20 cm −2 .&#xD;
The X-ray luminosity of the source was 2.23 × 10 30 ergs s −1 .</summary>
    <dc:date>2022-04-01T00:00:00Z</dc:date>
  </entry>
  <entry>
    <title>Meidcal image processing: denoising dynamic perfusion MRI (DCE-MRI) data using AI</title>
    <link rel="alternate" href="http://hdl.handle.net/123456789/2055" />
    <author>
      <name>Mishra, Akhil Ratan</name>
    </author>
    <id>http://hdl.handle.net/123456789/2055</id>
    <updated>2022-12-23T19:10:25Z</updated>
    <published>2022-04-01T00:00:00Z</published>
    <summary type="text">Title: Meidcal image processing: denoising dynamic perfusion MRI (DCE-MRI) data using AI
Authors: Mishra, Akhil Ratan
Abstract: Dynamic Contrast-Enhanced MRI (DCE-MRI) has been established as a non-invasive imaging&#xD;
technique which is extensively used to quantitatively evaluate tumour biology in many&#xD;
physiological and pathological cases. The dynamic scans are then used to quantify the&#xD;
permeability of the contrast agent to the Blood-Brain Barrier (BBB) by extracting the&#xD;
pharmacokinetic parameters. However, the DCE-MRI concentration curves (C(t)) are prone to&#xD;
Gaussian and Rician noise. In this study, an attempt is based to understand the variation of&#xD;
different Tracer Kinetic Parameters (TKP) at various noise levels. Further, state of the art deep&#xD;
learning-based denoising systems were trained to capture the different noise levels and&#xD;
characteristic shapes of the C(t) in an attempt to reduce the noise found in the real dataset. For&#xD;
training as clean signals (ground truth) are not available, the Generalized Tracer Kinetic Model&#xD;
(GTKM) with non-linear dynamics was used to generate pragmatic training data. The results&#xD;
of this study reveal the dependence of TKP on noise levels. It was also found that deep&#xD;
denoising systems were able to bring down the inherent noise in the C(t) curves from the Gray&#xD;
Matter and White Matter in the real dataset. This is validated by the improved Signal to Noise&#xD;
Ratio (SNR) and increase in the similarity index of the concentration curves of neighbouring&#xD;
voxels.</summary>
    <dc:date>2022-04-01T00:00:00Z</dc:date>
  </entry>
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