<?xml version="1.0" encoding="utf-8"?>
<journal>
<title>International Journal of Optics and Photonics</title>
<title_fa></title_fa>
<short_title>IJOP</short_title>
<subject>Basic Sciences</subject>
<web_url>http://ijop.ir</web_url>
<journal_hbi_system_id>1</journal_hbi_system_id>
<journal_hbi_system_user>admin</journal_hbi_system_user>
<journal_id_issn>1735-8590</journal_id_issn>
<journal_id_issn_online>2538-4007</journal_id_issn_online>
<journal_id_pii></journal_id_pii>
<journal_id_doi>10.61186/ijop</journal_id_doi>
<journal_id_iranmedex></journal_id_iranmedex>
<journal_id_magiran></journal_id_magiran>
<journal_id_sid></journal_id_sid>
<journal_id_nlai>1735-8590</journal_id_nlai>
<journal_id_science></journal_id_science>
<language>en</language>
<pubdate>
	<type>jalali</type>
	<year>1398</year>
	<month>10</month>
	<day>1</day>
</pubdate>
<pubdate>
	<type>gregorian</type>
	<year>2020</year>
	<month>1</month>
	<day>1</day>
</pubdate>
<volume>14</volume>
<number>1</number>
<publish_type>online</publish_type>
<publish_edition>1</publish_edition>
<article_type>fulltext</article_type>
<articleset>
	<article>


	<language>en</language>
	<article_id_doi></article_id_doi>
	<title_fa></title_fa>
	<title>Optical and Elecrtical Simulation of CH3NH3PbI3-based Perovskite Solar Cells</title>
	<subject_fa>عمومى</subject_fa>
	<subject>General</subject>
	<content_type_fa>پژوهشي</content_type_fa>
	<content_type>Research</content_type>
	<abstract_fa></abstract_fa>
	<abstract>Recently, organo&amp;ndash;metal halide perovskites have attracted much attention of the scientific community relating to their successful application in the absorber layer of low-cost solar cells. However, enough is known about the material and device properties, to realize that much remains to be learned.&lt;br&gt;
&lt;a name=&quot;OLE_LINK557&quot;&gt;&lt;/a&gt;&lt;a name=&quot;OLE_LINK556&quot;&gt;In this paper, the electrical and optical &lt;/a&gt;&lt;a name=&quot;OLE_LINK329&quot;&gt;&lt;/a&gt;&lt;a name=&quot;OLE_LINK328&quot;&gt;properties&lt;/a&gt; of perovskite solar cells are investigated &lt;a name=&quot;OLE_LINK551&quot;&gt;&lt;/a&gt;&lt;a name=&quot;OLE_LINK550&quot;&gt;using the COMSOL Multiphysics &lt;/a&gt;&lt;a name=&quot;OLE_LINK553&quot;&gt;&lt;/a&gt;&lt;a name=&quot;OLE_LINK552&quot;&gt;simulation program&lt;/a&gt;. It is a study of the influences &lt;a name=&quot;OLE_LINK327&quot;&gt;&lt;/a&gt;&lt;a name=&quot;OLE_LINK326&quot;&gt;of carrier diffusion length (L), &lt;/a&gt;&lt;a name=&quot;OLE_LINK358&quot;&gt;&lt;/a&gt;&lt;a name=&quot;OLE_LINK357&quot;&gt;dielectric constant (&lt;/a&gt;&amp;epsilon;&lt;sub&gt;r&lt;/sub&gt;), the valence band offset (VBO) of absorber/hole transport materials (HTM) and illumination intensity on fill factor (FF), short-circuit current density(J&lt;sub&gt;SC&lt;/sub&gt;), performance (PCE), and open-circuit voltage(V&lt;sub&gt;OC&lt;/sub&gt;). Also, J-V characteristics are calculated for diff&lt;a name=&quot;OLE_LINK335&quot;&gt;&lt;/a&gt;&lt;a name=&quot;OLE_LINK334&quot;&gt;eren&lt;/a&gt;t &amp;epsilon;&lt;sub&gt;r&lt;/sub&gt; values. The simulation results point to the great dependence of efficiency on the carrier diffusion length of absorber layers. It is shown that, to obtain a high rate of efficiency, the relative permittivity should not be higher than 45.&lt;a name=&quot;OLE_LINK77&quot;&gt;&lt;/a&gt;&lt;br&gt;
&amp;nbsp;</abstract>
	<keyword_fa></keyword_fa>
	<keyword>Perovskite solar cells, Fill Factor, Power Conversion Efficiency, Simulation.</keyword>
	<start_page>57</start_page>
	<end_page>66</end_page>
	<web_url>http://ijop.ir/browse.php?a_code=A-10-518-3&amp;slc_lang=en&amp;sid=1</web_url>


<author_list>
	<author>
	<first_name>Elham</first_name>
	<middle_name></middle_name>
	<last_name>Karimi</last_name>
	<suffix></suffix>
	<first_name_fa></first_name_fa>
	<middle_name_fa></middle_name_fa>
	<last_name_fa></last_name_fa>
	<suffix_fa></suffix_fa>
	<email></email>
	<code>10031947532846003122</code>
	<orcid>10031947532846003122</orcid>
	<coreauthor>No</coreauthor>
	<affiliation>Department of Physics, Faculty of Physics, University of Kashan, Kashan, Iran</affiliation>
	<affiliation_fa></affiliation_fa>
	 </author>


	<author>
	<first_name>Seyed Mohamad Bagher</first_name>
	<middle_name></middle_name>
	<last_name>Ghorashi</last_name>
	<suffix></suffix>
	<first_name_fa></first_name_fa>
	<middle_name_fa></middle_name_fa>
	<last_name_fa></last_name_fa>
	<suffix_fa></suffix_fa>
	<email>mghorashi@kashanu.ac.ir</email>
	<code>10031947532846003123</code>
	<orcid>10031947532846003123</orcid>
	<coreauthor>Yes
</coreauthor>
	<affiliation>Department of Physics, Faculty of Physics, University of Kashan, Kashan, Iran</affiliation>
	<affiliation_fa></affiliation_fa>
	 </author>


	<author>
	<first_name>Maryam</first_name>
	<middle_name></middle_name>
	<last_name>Hashemi</last_name>
	<suffix></suffix>
	<first_name_fa></first_name_fa>
	<middle_name_fa></middle_name_fa>
	<last_name_fa></last_name_fa>
	<suffix_fa></suffix_fa>
	<email></email>
	<code>10031947532846003124</code>
	<orcid>10031947532846003124</orcid>
	<coreauthor>No</coreauthor>
	<affiliation>Department of Physics, Faculty of Physics, University of Kashan, Kashan, Iran</affiliation>
	<affiliation_fa></affiliation_fa>
	 </author>


</author_list>


	</article>
</articleset>
</journal>
