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<article xlink="http://www.w3.org/1999/xlink" dtd-version="1.0" article-type="general-sciences" lang="en"><front><journal-meta><journal-id journal-id-type="publisher">IJCRR</journal-id><journal-id journal-id-type="nlm-ta">I Journ Cur Res Re</journal-id><journal-title-group><journal-title>International Journal of Current Research and Review</journal-title><abbrev-journal-title abbrev-type="pubmed">I Journ Cur Res Re</abbrev-journal-title></journal-title-group><issn pub-type="ppub">2231-2196</issn><issn pub-type="opub">0975-5241</issn><publisher><publisher-name>Radiance Research Academy</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="publisher-id">2559</article-id><article-id pub-id-type="doi"/><article-id pub-id-type="doi-url">http://dx.doi.org/10.31782/IJCRR.2018.3235</article-id><article-categories><subj-group subj-group-type="heading"><subject>General Sciences</subject></subj-group></article-categories><title-group><article-title>Analysis of Highest Occupied and Lowest Unoccupied Molecular Orbitsl on Harmaline&#13;
</article-title></title-group><contrib-group><contrib contrib-type="author"><name><surname>ajalakshmi</surname><given-names>R</given-names></name></contrib><contrib contrib-type="author"><name><surname>Divya</surname><given-names/></name></contrib></contrib-group><pub-date pub-type="ppub"><day>14</day><month>11</month><year>2018</year></pub-date><volume>1)</volume><issue/><fpage>32</fpage><lpage>35</lpage><permissions><copyright-statement>This article is copyright of Popeye Publishing, 2009</copyright-statement><copyright-year>2009</copyright-year><license license-type="open-access" href="http://creativecommons.org/licenses/by/4.0/"><license-p>This is an open-access article distributed under the terms of the Creative Commons Attribution (CC BY 4.0) Licence. You may share and adapt the material, but must give appropriate credit to the source, provide a link to the licence, and indicate if changes were made.</license-p></license></permissions><abstract><p>Harmaline belonging to a family of harmala is a fluorescent psychoactive indole alkaloid. The FTIR and FT-Raman spectra of Harmaline have been recorded in region 4000__ampersandsignndash;400 cm-1 and 4,000__ampersandsignndash;100 cm-1 respectively. The experimental frequencies recorded are compared with vibration frequencies calculated using Gaussian software by employing HF and DFT functional at B3LYP/6-31G(d,p) basis set. The electronic properties of the molecule have been studied by recording UV__ampersandsignndash;Visible spectrum of the compound. Also, highest occupied (HOMO) and lowest unoccupied molecular orbital (LUMO) energies have been calculated at DFT/B3LYP/6-31 G (d,p) level. These calculations showed that there exists energy transfer in the molecule. Mulliken population analysis and thermodynamic properties of title compound have been analyzed and tabulated.&#13;
</p></abstract><kwd-group><kwd>Harmaline</kwd><kwd> FTIR</kwd><kwd> FT-RAMAN</kwd><kwd> HF</kwd><kwd> DFT</kwd><kwd> HOMO-LUMO</kwd></kwd-group></article-meta></front></article>
