{"id":1913,"date":"2015-07-05T21:56:53","date_gmt":"2015-07-06T04:56:53","guid":{"rendered":"http:\/\/physikon.net\/?p=1913"},"modified":"2022-06-22T09:50:53","modified_gmt":"2022-06-22T16:50:53","slug":"1913","status":"publish","type":"post","link":"http:\/\/physikon.net\/?p=1913","title":{"rendered":"The Superconducting Transition Temperatures of FeN<sub>1+x<\/sub>Se<sub>1-y<\/sub>, Fe<sub>1+x<\/sub>Se<sub>1-y<\/sub>Te<sub>y<\/sub> and (K\/Rb\/Cs)<sub>z<\/sub>Fe<sub>2-x<\/sub>Se<sub>2<\/sub>"},"content":{"rendered":"<p><!--more--><\/p>\n<hr \/>\n<p style=\"text-align: justify;\"><strong>The Superconducting Transition Temperatures of Fe<sub>1+x<\/sub>Se<sub>1-y<\/sub>, Fe<sub>1+x<\/sub>Se<sub>1-y<\/sub>Te<sub>y<\/sub> and (K\/Rb\/Cs)<sub>z<\/sub>Fe<sub>2-x<\/sub>Se<sub>2<\/sub>)<\/strong>, D. R. Harshman and A. T. Fiory [<a href=\"https:\/\/doi.org\/10.48550\/arXiv.1202.0329\">arXiv<\/a>]\n<p style=\"text-align: justify;\">In a recent contribution to this journal, it was shown that the transition temperatures of optimal high-<em>T<\/em>c compounds obey the algebraic relation, <em>T<\/em><sub>C0<\/sub> = k<sub>B<\/sub><sup>\u20131<\/sup>\u03b2\/\u2113\u03b6, where \u2113 is related to the mean spacing between interacting charges in the layers, \u03b6 is the distance between interacting electronic layers, \u03b2 is a universal constant and k<sub>B<\/sub> is Boltzmann\u2019s constant. The equation was derived assuming pairing based on interlayer Coulomb interactions between physically separated charges. This theory was initially validated for 31 compounds from five different high-<em>T<\/em><sub>C<\/sub> families (within an accuracy of \u00b11.37 K). Herein we report the addition of Fe<sub>1+x<\/sub>Se<sub>1\u2013y<\/sub> and Fe<sub>1+x<\/sub>Se<sub>1\u2013y<\/sub>Te<sub>y<\/sub> (both optimized under pressure) and A<sub>z<\/sub>Fe<sub>2\u2013x<\/sub>Se<sub>2<\/sub> (for A = K, Rb, or Cs) to the growing list of Coulomb-mediated superconducting compounds in which T<sub>C0<\/sub> is determined by the above equation. Doping in these materials is accomplished through the introduction of excess Fe and\/or Se deficiency, or a combination of alkali metal and Fe vacancies. Consequently, a very small number of vacancies or interstitials can induce a superconducting state with a substantial transition temperature. The confirmation of the above equation for these Se-based Fe chalcogenides increases to six the number of superconducting families for which the transition temperature can be accurately predicted.<\/p>\n<p style=\"text-align: justify;\">\n<table id=\"tablepress-14\" class=\"tablepress tablepress-id-14\">\n<tbody class=\"row-hover\">\n<tr class=\"row-1\">\n\t<td class=\"column-1\"><a href=\"http:\/\/physikon.net\/wp-content\/uploads\/2015\/05\/CTTKFS_Figure1.jpg\"><img loading=\"lazy\" decoding=\"async\" src=\"http:\/\/physikon.net\/wp-content\/uploads\/2015\/05\/CTTKFS_Figure1-300x198.jpg\" alt=\"CTTKFS_Figure1\" width=\"300\" height=\"198\" class=\"alignright size-medium wp-image-1401\" srcset=\"http:\/\/physikon.net\/wp-content\/uploads\/2015\/05\/CTTKFS_Figure1.jpg 300w, http:\/\/physikon.net\/wp-content\/uploads\/2015\/05\/CTTKFS_Figure1-227x150.jpg 227w, http:\/\/physikon.net\/wp-content\/uploads\/2015\/05\/CTTKFS_Figure1-150x99.jpg 150w\" sizes=\"auto, (max-width: 300px) 100vw, 300px\" \/><\/a><br \/>\n<p align=\"justify\">Schematic diagram of (a) Fe<sub>1+x<\/sub>Se<sub>1\u2013y<\/sub> and (b) K<sub>x<\/sub>Fe<sub>2\u2013y<\/sub>Se<sub>2<\/sub>, as projected views along their [110] directions (linear densities of tetrahedrally-coordinated Fe are twice those of Se), illustrating the structures of the type I and type II reservoirs, the periodicity d and the interaction distance &zeta;.  Vacancies and excess atoms are not shown.<\/p><\/td>\n<\/tr>\n<tr class=\"row-2\">\n\t<td class=\"column-1\"><a href=\"http:\/\/physikon.net\/wp-content\/uploads\/2015\/05\/CTTKFS_Figure2.jpg\"><img loading=\"lazy\" decoding=\"async\" src=\"http:\/\/physikon.net\/wp-content\/uploads\/2015\/05\/CTTKFS_Figure2-300x271.jpg\" alt=\"CTTKFS_Figure2\" width=\"300\" height=\"271\" class=\"alignleft size-medium wp-image-1402\" srcset=\"http:\/\/physikon.net\/wp-content\/uploads\/2015\/05\/CTTKFS_Figure2.jpg 300w, http:\/\/physikon.net\/wp-content\/uploads\/2015\/05\/CTTKFS_Figure2-166x150.jpg 166w, http:\/\/physikon.net\/wp-content\/uploads\/2015\/05\/CTTKFS_Figure2-150x136.jpg 150w\" sizes=\"auto, (max-width: 300px) 100vw, 300px\" \/><\/a><br \/>\n<p align=\"justify\">The optimal superconducting transition temperature <em>T<\/em><sub>C0<\/sub> plotted against (\u2113&zeta;)<sup>-1<\/sup>, where \u2113 is the mean in-plane distance between participating charges and &zeta; is the distance between interacting layers.  The five 11 and 122 Fe chalcogenides (solid symbols) are compared to the 1111 and 122 Fe pnictides (open triangles) and the remainder of the thirty-six compounds (open circles), exhibiting behaviors in agreement with theory, represented by solid line.<\/p><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<!-- #tablepress-14 from cache -->\n<p style=\"text-align: justify;\">D. R. Harshman and A. T. Fiory, <a href=\"https:\/\/doi.org\/10.1088\/0953-8984\/24\/13\/135701\">J. Phys.: Condens. Matter <strong>24<\/strong>, 135701 (2012)<\/a>.<\/p>\n<hr \/>\n","protected":false},"excerpt":{"rendered":"","protected":false},"author":1,"featured_media":1402,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[9,8],"tags":[],"class_list":["post-1913","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-high-tc-superconductivity","category-high-tc-theory"],"_links":{"self":[{"href":"http:\/\/physikon.net\/index.php?rest_route=\/wp\/v2\/posts\/1913","targetHints":{"allow":["GET"]}}],"collection":[{"href":"http:\/\/physikon.net\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"http:\/\/physikon.net\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"http:\/\/physikon.net\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"http:\/\/physikon.net\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=1913"}],"version-history":[{"count":13,"href":"http:\/\/physikon.net\/index.php?rest_route=\/wp\/v2\/posts\/1913\/revisions"}],"predecessor-version":[{"id":7704,"href":"http:\/\/physikon.net\/index.php?rest_route=\/wp\/v2\/posts\/1913\/revisions\/7704"}],"wp:featuredmedia":[{"embeddable":true,"href":"http:\/\/physikon.net\/index.php?rest_route=\/wp\/v2\/media\/1402"}],"wp:attachment":[{"href":"http:\/\/physikon.net\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=1913"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"http:\/\/physikon.net\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=1913"},{"taxonomy":"post_tag","embeddable":true,"href":"http:\/\/physikon.net\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=1913"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}