<?xml version="1.0" encoding="UTF-8"?>
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  <title>DSpace Community: Associate Professor and Head, Zonuam, Aizawl</title>
  <link rel="alternate" href="http://pucir.inflibnet.ac.in:8080/jspui/handle/123456789/224" />
  <subtitle>Associate Professor and Head, Zonuam, Aizawl</subtitle>
  <id>http://pucir.inflibnet.ac.in:8080/jspui/handle/123456789/224</id>
  <updated>2026-04-30T21:10:15Z</updated>
  <dc:date>2026-04-30T21:10:15Z</dc:date>
  <entry>
    <title>Casimir wormhole solutions in 𝑓(𝑅,𝑚 ) gravity</title>
    <link rel="alternate" href="http://pucir.inflibnet.ac.in:8080/jspui/handle/123456789/1058" />
    <author>
      <name>Lalvohbika, J</name>
    </author>
    <id>http://pucir.inflibnet.ac.in:8080/jspui/handle/123456789/1058</id>
    <updated>2025-10-21T06:18:50Z</updated>
    <published>2024-03-01T00:00:00Z</published>
    <summary type="text">Title: Casimir wormhole solutions in 𝑓(𝑅,𝑚 ) gravity
Authors: Lalvohbika, J
Abstract: In this paper, we study the Casimir effect on the wormhole geometry in 𝑓(𝑅,𝑚&#xD;
) gravity. We&#xD;
derive the field equations for the generic 𝑓(𝑅,𝑚&#xD;
) function by assuming static and spherically&#xD;
symmetric Morris–Thorne wormhole metric. Then we consider two non-linear 𝑓(𝑅,𝑚&#xD;
) models,&#xD;
specifically, 𝑓(𝑅,𝑚&#xD;
) = 𝑅&#xD;
2&#xD;
+&#xD;
𝛽&#xD;
𝑚 and 𝑓(𝑅,𝑚&#xD;
) = 𝑅&#xD;
2&#xD;
+(1+𝛼𝑚&#xD;
)𝑚 where 𝛼 and 𝛽 are free parameters.&#xD;
We derive the shape functions for wormholes by utilizing the Casimir effect and examining&#xD;
their existence. Subsequently, we analyse the obtained wormhole solutions for each scenario,&#xD;
assessing the energy conditions at the wormhole throat with a radius of 𝑟0&#xD;
. Our findings reveal&#xD;
that for some arbitrary quantities, there is a violation of classical energy conditions at the&#xD;
wormhole throat. Additionally, we delve into the behaviour of the equation of state (EoS) for&#xD;
each case. Furthermore, we explore the stability of the Casimir effect wormhole solutions by&#xD;
employing the generalized Tolman–Oppenheimer–Volkoff (TOV) equation. Finally, we utilize&#xD;
the volume integral quantifier to determine the amount of exotic matter required near the&#xD;
wormhole throat for both models.</summary>
    <dc:date>2024-03-01T00:00:00Z</dc:date>
  </entry>
  <entry>
    <title>Scattering of qSH-waves from a corrugated interface between two dissimilar nematic elastomers</title>
    <link rel="alternate" href="http://pucir.inflibnet.ac.in:8080/jspui/handle/123456789/1057" />
    <author>
      <name>Lalvohbika, J</name>
    </author>
    <id>http://pucir.inflibnet.ac.in:8080/jspui/handle/123456789/1057</id>
    <updated>2025-10-21T06:16:31Z</updated>
    <published>2020-04-15T00:00:00Z</published>
    <summary type="text">Title: Scattering of qSH-waves from a corrugated interface between two dissimilar nematic elastomers
Authors: Lalvohbika, J
Abstract: This paper aims to investigate the reflection and transmission phenomena of elastic waves due to incident qSH-wave at a corrugated&#xD;
interface between two different nematic elastomer half-spaces. The&#xD;
expression of the phase velocity for shear harmonic wave is derived&#xD;
and observed that this phase velocity depends on the angle of&#xD;
propagation. There exist irregularly reflected and transmitted waves&#xD;
besides the regular waves due to undulated nature of the interface whose nth spectrum is related through Spectrum theorem. The&#xD;
amplitude ratios for various reflected and transmitted waves are&#xD;
derived using boundary conditions. The ratios corresponding to an&#xD;
irregular waves arefound to befunctions of the incident angle, elastic&#xD;
constants, relaxation times, corrugation and frequency parameters.&#xD;
The energy distribution, and hence the energy ratios due to various reflected and transmitted waves are also obtained. It is observed&#xD;
that the sum of all energy ratios is approximately unity at each value&#xD;
of incident angle which ensures the law of conservation of energy&#xD;
at the interface. A particular case, z = d cos px has been performed&#xD;
to validate the present study for the amplitude and energy ratios.&#xD;
Graphs are plotted for these ratios at different values of corrugation&#xD;
and frequency parameters to discuss their effects.</summary>
    <dc:date>2020-04-15T00:00:00Z</dc:date>
  </entry>
  <entry>
    <title>THESIS SUBMITTED IN PARTIAL FULFILMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY J. LALVOHBIKA</title>
    <link rel="alternate" href="http://pucir.inflibnet.ac.in:8080/jspui/handle/123456789/783" />
    <author>
      <name>Lalvohbika, J</name>
    </author>
    <id>http://pucir.inflibnet.ac.in:8080/jspui/handle/123456789/783</id>
    <updated>2024-06-18T06:30:43Z</updated>
    <published>2021-01-01T00:00:00Z</published>
    <summary type="text">Title: THESIS SUBMITTED IN PARTIAL FULFILMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY J. LALVOHBIKA
Authors: Lalvohbika, J
Abstract: THESIS SUBMITTED IN PARTIAL FULFILMENT OF&#xD;
THE REQUIREMENTS FOR THE DEGREE OF DOCTOR&#xD;
OF PHILOSOPHY&#xD;
J. LALVOHBIKA</summary>
    <dc:date>2021-01-01T00:00:00Z</dc:date>
  </entry>
  <entry>
    <title>SCATTERING OF ELASTIC WAVES FROM A CORRUGATED INTERFACE</title>
    <link rel="alternate" href="http://pucir.inflibnet.ac.in:8080/jspui/handle/123456789/782" />
    <author>
      <name>Lalvohbika, J</name>
    </author>
    <author>
      <name>Lalvohbika, J</name>
    </author>
    <id>http://pucir.inflibnet.ac.in:8080/jspui/handle/123456789/782</id>
    <updated>2024-06-18T06:27:18Z</updated>
    <published>2014-01-01T00:00:00Z</published>
    <summary type="text">Title: SCATTERING OF ELASTIC WAVES FROM A CORRUGATED INTERFACE; SCATTERING OF ELASTIC WAVES FROM A CORRUGATED INTERFACE
Authors: Lalvohbika, J; Lalvohbika, J
Abstract: THESIS SUBMITTED IN PARTIAL FULFILMENT OF&#xD;
THE REQUIREMENTS FOR THE DEGREE OF DOCTOR&#xD;
OF PHILOSOPHY&#xD;
J. LALVOHBIKA</summary>
    <dc:date>2014-01-01T00:00:00Z</dc:date>
  </entry>
</feed>

