<?xml version="1.0"?>
<records>
  <record>
    <language>eng</language>
    <publisher>Ansari Education and Research Society</publisher>
    <journalTitle>Journal of Ultra Scientist of Physical Sciences</journalTitle>
    <issn/>
    <eissn/>
    <publicationDate>March 2023</publicationDate>
    <volume>35</volume>
    <issue>2</issue>
    <startPage>16</startPage>
    <endPage>23</endPage>
    <doi>http://dx.doi.org/10.22147/jusps-B/350201</doi>
    <publisherRecordId>1537</publisherRecordId>
    <documentType>article</documentType>
    <title language="eng">Inflationary Scenario in Bianchi Type &#x2013; V Cosmological Model with Bulk Viscosity in General Relativity</title>
    <authors>
      <author>
        <name>JYOTI SINGH</name>
        <affiliationId>1</affiliationId>
      </author>
      <author>
        <name>ATUL TYAGI</name>
        <affiliationId>1</affiliationId>
      </author>
      <author>
        <name>JAIPAL SINGH</name>
        <affiliationId>2</affiliationId>
      </author>
      <author>
        <name>DHIRENDRA CHHAJED</name>
        <affiliationId>1</affiliationId>
      </author>
    </authors>
    <affiliationsList>
      <affiliationName affiliationId="1">Department of Mathematics and Statistics, University College of Science, MLS University, Udaipur- 313001 (India)</affiliationName>
      <affiliationName affiliationId="2">Department of Basic Science Mathematics, CTAE, College MPUAT University, Udaipur- 313001 (India)</affiliationName>
    </affiliationsList>
    <abstract language="eng">&lt;p&gt;In present paper we have investigated the inflationary scenario in Bianchi Type V cosmological model under the effect of bulk viscosity in general relativity. To get deterministic model of the universe, we assume the shear (&lt;img alt="sigma" src="https://latex.codecogs.com/gif.latex?%5Csigma" /&gt;) is proportional to the expansion (&lt;img alt="theta" src="https://latex.codecogs.com/gif.latex?%5Ctheta" /&gt;) by which a condition A&lt;sub&gt;1&lt;/sub&gt; = (A&lt;sub&gt;2&lt;/sub&gt;A&lt;sub&gt;3&lt;/sub&gt;)&lt;sup&gt;n&lt;/sup&gt;&amp;nbsp;between metric potentials is obtained. We consider the region is flat which leads to the scalar potential&lt;em&gt; V&lt;/em&gt;(&lt;img alt="phi" src="https://latex.codecogs.com/gif.latex?%5Cphi" /&gt;) is constant. We found the spatial volume increases with time, which represent the inflationary scenario in the model. Some physical and geometrical properties of the model are also discussed in detail. The model is found to be compatible with the results of recent observations.&lt;/p&gt;&#xD;
</abstract>
    <fullTextUrl format="html">https://ultraphysicalsciences.org/paper/1537/</fullTextUrl>
    <keywords>
      <keyword language="eng">Bianchi Type-V,</keyword>
    </keywords>
    <keywords>
      <keyword language="eng">bulk viscous fluid</keyword>
    </keywords>
    <keywords>
      <keyword language="eng">inflationary</keyword>
    </keywords>
    <keywords>
      <keyword language="eng">general relativity</keyword>
    </keywords>
  </record>
</records>
