<?xml version="1.0" encoding="UTF-8"?><feed xmlns="http://www.w3.org/2005/Atom" xmlns:dc="http://purl.org/dc/elements/1.1/">
<title>Mathematcics</title>
<link href="http://103.99.128.19:8080/xmlui/handle/123456789/5" rel="alternate"/>
<subtitle>Mathematics</subtitle>
<id>http://103.99.128.19:8080/xmlui/handle/123456789/5</id>
<updated>2026-10-04T07:31:50Z</updated>
<dc:date>2026-10-04T07:31:50Z</dc:date>
<entry>
<title>SIMULATION OF HEAT TRANSFER  ENHANCEMENT IN A PIPE USING RECTANGULAR  CUT TWISTED TAPE INSERT: A FEM APPROACH</title>
<link href="http://103.99.128.19:8080/xmlui/handle/123456789/602" rel="alternate"/>
<author>
<name>Anika, Onamika Ibnath</name>
</author>
<author>
<name>ID :, 21MMATH009F</name>
</author>
<id>http://103.99.128.19:8080/xmlui/handle/123456789/602</id>
<updated>2026-10-04T06:20:38Z</updated>
<published>2025-04-08T00:00:00Z</published>
<summary type="text">SIMULATION OF HEAT TRANSFER  ENHANCEMENT IN A PIPE USING RECTANGULAR  CUT TWISTED TAPE INSERT: A FEM APPROACH
Anika, Onamika Ibnath; ID :, 21MMATH009F
A simulation analysis has been conducted to investigate heat transfer enhancement &#13;
using rectangular-cut twisted tape inserts in a U-shaped pipe. Numerical simulations &#13;
have also been carried out for a plain tube and a tube with smooth twisted tape (TT) &#13;
inserts, and the results have been compared across three configurations: rectangular-cut &#13;
TT inserts, smooth TT inserts, and the plain tube. The analysis has utilized a U-bend &#13;
pipe with a length of 1935.6 mm and an inner diameter of 26.6 mm. For non-isothermal &#13;
turbulent flow, water has been selected as the working fluid, and the Reynolds number &#13;
(Re) range has been considered from 5319.4 to 17288.05. The rectangular-cut twisted &#13;
tape inserts have demonstrated superior heat transfer performance compared to the other &#13;
two configurations due to enhanced fluid mixing in the turbulent flow regime. In this &#13;
study, the dimensionless Nusselt number (Nu) has consistently been higher for the &#13;
rectangular-cut twisted tape configuration and has shown a gradual increase with rising &#13;
Reynolds numbers. The results have also indicated improved thermal performance (ɳ), &#13;
with a thermal performance factor of 1.04 and favorable friction factor values for the &#13;
pipe fitted with rectangular cut twisted tape inserts.
A Master of Philosophy (M.Phil.) Thesis in Mathematics  Department at Chittagong University of Engineering and Technology (CUET).
</summary>
<dc:date>2025-04-08T00:00:00Z</dc:date>
</entry>
<entry>
<title>NUMERICAL INVESTIGATIONOFNONLINEAR ACOUSTICWAVEPHENOMENA INSTRONGLYAND WEAKLYCOUPLEDPLASMAS</title>
<link href="http://103.99.128.19:8080/xmlui/handle/123456789/599" rel="alternate"/>
<author>
<name>Islam, Md. Nazrul</name>
</author>
<id>http://103.99.128.19:8080/xmlui/handle/123456789/599</id>
<updated>2026-10-04T06:19:28Z</updated>
<published>2025-07-17T00:00:00Z</published>
<summary type="text">NUMERICAL INVESTIGATIONOFNONLINEAR ACOUSTICWAVEPHENOMENA INSTRONGLYAND WEAKLYCOUPLEDPLASMAS
Islam, Md. Nazrul
This thesis investigates nonlinear acoustic wave phenomena in both strongly and weakly&#13;
coupled collisionless unmagnetized plasmas using analytical and numerical methods. By&#13;
developing mathematical models for different plasma environments, the study employs the&#13;
reductive perturbation technique (RPT) to derive nonlinear evolution equations (NLEEs).&#13;
These equations are then used to analyze the propagation of shock waves, solitons, and&#13;
periodic waves in various plasma configurations.&#13;
In Chapter 2, Burgers equations involving quadratic, cubic, and combined&#13;
quadratic-cubic nonlinearities are derived for a coupled complex plasma system consisting&#13;
of Boltzmann-distributed electrons, nonthermal ions, and charged dust particles. The&#13;
generalized Riccati equation mapping method (GREMM) is employed to obtain both shock&#13;
and oscillatory wave solutions from these equations, while parametric effects on wave&#13;
characteristics are systematically examined.&#13;
Chapter 3 investigates heavy ion-acoustic shock waves (HIASWs) in a plasma&#13;
comprising inertial heavy ions, Maxwellian light ions, and (α,q)-distributed electrons, by&#13;
deriving the Burgers, modified Burgers, and mixed modified Burgers equations. The study&#13;
presents stationary shock wave solutions for these equations and examines how plasma&#13;
parameters influence shock wave characteristics.&#13;
Chapter 4 investigates the dust acoustic (DA) shock wave phenomena in an strongly&#13;
coupled dusty plasma. By deriving Burgers equations with quadratic, cubic, and quartic&#13;
nonlinearities, we analyze shock wave behavior near critical values (CVs) and super-critical&#13;
values (SCVs), revealing how polarization force and coupling parameter modifies shock&#13;
wave excitations.&#13;
Chapter 5 analyzes heavy ion-acoustic (HIA) solitons and dressed solitons in&#13;
weakly/strongly coupled plasmas with nonthermal electrons.&#13;
Chapter 6 advances the Chapter 3 framework by examining HIASWs near CVs and&#13;
SCVs, deriving a non-integrable NLEE with combined cubic-quartic nonlinearities that&#13;
necessitates numerical solution via Runge-Kutta-Fehlberg analysis.&#13;
Thus, the thesis enhances understanding of nonlinear coherent structures observed in&#13;
various space and astrophysical environments.
A Doctor of Philosophy (Ph.D.) Thesis in Mathematics Department at Chittagong University of Engineering and Technology (CUET).
</summary>
<dc:date>2025-07-17T00:00:00Z</dc:date>
</entry>
<entry>
<title>DESIGNING CONTROL SCHEMS FOR  CHAOTIC SYSTEMS VIA SLIDING  MODE CONTROL</title>
<link href="http://103.99.128.19:8080/xmlui/handle/123456789/589" rel="alternate"/>
<author>
<name>AFROJA, AFSANA</name>
</author>
<author>
<name>ID:, 21MMATH002P</name>
</author>
<id>http://103.99.128.19:8080/xmlui/handle/123456789/589</id>
<updated>2026-09-10T04:24:31Z</updated>
<published>2025-07-07T00:00:00Z</published>
<summary type="text">DESIGNING CONTROL SCHEMS FOR  CHAOTIC SYSTEMS VIA SLIDING  MODE CONTROL
AFROJA, AFSANA; ID:, 21MMATH002P
Among various robust control methods, Sliding Mode Control (SMC) has attracted &#13;
considerable interest in theoretical research due to its unique features. SMC is well known &#13;
for its robustness to matched and bounded uncertainties, reduction in the order of the &#13;
system during the sliding phase, simplified decoupling of system dynamics, and its ability &#13;
to achieve zero steady-state error. These characteristics make SMC a powerful tool in &#13;
designing control systems for uncertain and nonlinear environments. &#13;
This thesis presents a comprehensive study on the control and synchronization of chaotic &#13;
systems, focusing on the Modified Lorenz System (MLS) and the Liu financial dynamical &#13;
system. Chaotic behavior, with its sensitivity to initial conditions, presents major &#13;
challenges in nonlinear control. Sliding Mode Control (SMC) is applied to coupled MLS &#13;
to ensure robust synchronization through a designed sliding surface and control law, with &#13;
convergence proven via Lyapunov stability and validated through numerical simulations. &#13;
In the Liu financial system, both SMC and Passive Control (PC) are implemented and &#13;
compared. While SMC provides rapid synchronization (within &#55349;&#56417; ≥ 1, error reduced from &#13;
5.67 to 0.02), PC achieves synchronization more gradually (within &#55349;&#56417; ≤ 13, error reduced &#13;
from 6.21 to 0.03) using a simpler, single-controller strategy. The results highlight key &#13;
trade-offs between speed, robustness, and implementation complexity, offering valuable &#13;
insights into managing chaos in nonlinear and financial systems. &#13;
These limitations have motivated ongoing research aimed at improving SMC design. The &#13;
core challenge remains how to develop a simple yet effective sliding mode control &#13;
technique that retains its robustness and zero-error tracking while minimizing chattering &#13;
and relaxing the need for precise uncertainty bounds.
A Master of Philosophy (M.Phil.) Thesis in Mathematics  Department at Chittagong University of Engineering and Technology (CUET).
</summary>
<dc:date>2025-07-07T00:00:00Z</dc:date>
</entry>
<entry>
<title>ISOTROPIC SOLUTION OF EINSTEIN’S EQUATIONS ONTHE FLUIDSPHERE</title>
<link href="http://103.99.128.19:8080/xmlui/handle/123456789/567" rel="alternate"/>
<author>
<name>HOSSAIN, MD.IMRAN</name>
</author>
<author>
<name>ID:, 21MMATH005</name>
</author>
<id>http://103.99.128.19:8080/xmlui/handle/123456789/567</id>
<updated>2026-09-06T05:37:11Z</updated>
<published>2025-03-20T00:00:00Z</published>
<summary type="text">ISOTROPIC SOLUTION OF EINSTEIN’S EQUATIONS ONTHE FLUIDSPHERE
HOSSAIN, MD.IMRAN; ID:, 21MMATH005
This thesis investigates the theoretical framework of spherically symmetric perfect&#13;
fluid spheres within the realm of general relativity. Our work seeks exact solutions to the&#13;
Einstein field equations thereby facilitating a better knowledge of minuscule objects. The&#13;
thesis begins by examining the fundamental aspects of special relativity, including the&#13;
Lorentz transformations and the structure of spacetime. We then explore general relativity,&#13;
with an eye towards the Einstein field equations and the geometric justification of gravity.&#13;
Examining matter dispersion in astrophysical systems depends on first looking at the&#13;
behavior of ideal fluids.&#13;
The thesis delves into the intricacies of the Einstein field equations and their application&#13;
to spacetimes with spherical symmetry. The key achievement of the research is the&#13;
formulation of new exact solutions for static spherically symmetric ideal fluid spheres.&#13;
Implementing two techniques in the context of static spherically symmetric ideal fluid line&#13;
elements, we develop two new approaches that validate their characteristics and ensure&#13;
that they satisfy Buchdhal criteria.&#13;
The physical characteristics and possible astrophysical implications of these solutions are&#13;
thoroughly investigated. Combining the ideas of general relativity with the simplified&#13;
model of perfect fluids helps this work provide new understanding on the interactions&#13;
between compact objects and their gravitational interactions.
An M.Phil. Thesis in Mathematics Department at Chittagong University of Engineering and Technology (CUET).
</summary>
<dc:date>2025-03-20T00:00:00Z</dc:date>
</entry>
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