www.wikidata.uk-ua.nina.az
Ochikuyetsya sho seriya superaktinoyidiv angl superactinide bude mistiti elementi vid 121 do 157 U seriyi superaktinoyidiv 7d3 2 8p1 2 6f5 2 ta 5g7 2 elektronni obolonki povinni zapovnyuvatisya odnochasno ce stvoryuye duzhe skladni situaciyi tak silno tak sho povni ta tochni rozrahunki CCSD buli vikonani lishe dlya elementiv 121 ta 122 Pershij superaktinoyid Unbiunij element 121 povinen buti konzhenerom lantanu ta aktiniyu i maye mati podibni vlastivosti jogo osnovnij stan okislennya maye buti 3 hocha blizkist energetichnih rivniv valentnih orbitalej mozhe dozvoliti vishi stadiyi okislennya yak i v elementah 119 i 120 Relyativistska stabilizaciya pidsistemi 8p povinna sprichiniti konfiguraciyu valentnih elektron 8s28p1 dlya elementa 121 na vidminu vid konfiguracij ds2 lantanu ta aktiniyu Peredbachayetsya sho jogo persha energiya ionizaciyi stanovitime 429 4 kDzh mol sho nizhche nizh u vsih vidomih elementah za vinyatkom kaliyu rubidiyu ceziyu ta franciyu i luzhnih metaliv ce znachennya she nizhche nizh u periodu 8 luzhnogo metalu ununenniyu 463 kDzh mol Analogichnim chinom nastupnij superaktinid unbibij element 122 mozhe buti konzhenerom ceriyu ta toriyu osnovnij stan okislennya yakogo stanovit 4 ale vin matime valentnu elektronnu konfiguraciyu 7d18s28p1 na vidminu vid konfiguraciyi 6d27s2 toriyu Otzhe jogo persha energiya ionizaciyi bula b menshoyu nizh u toriyu Th 6 3 eV Ubb 5 6 eV cherez menshu energiyu vidrivu 8b1 2 elektrona unbibiyu nizh 6d elektrona toriyu U pershih kilkoh superaktinidah energiyi zv yazuvannya dodankovih elektroniv peredbachayutsya buti dosit malimi i takimi shob voni mogli vtratiti vsi svoyi valentni elektroni napriklad unbigeksij element 126 mozhe legko utvoriti stanu okislennya 8 i navit mozhlivi stadiyi okislennya navit dlya nastupnih kilkoh elementiv Takozh peredbachayetsya sho unbigeksij viyavlyaye cilij ryad inshih stupeniv okisnennya ostanni rozrahunki pokazali sho stabilnij monoftorid UbhF mozhe viyavitisya mozhlivim zavdyaki vzayemodiyi z yednannya 5g orbitali na unibigeksiyi ta 2p orbitali ftoru Inshi peredbachuvani stupeni okislennya vklyuchayut 2 4 ta 6 Ochikuyetsya sho SO 4 stane najposhirenishim stanom okislennya nebigeksiyu Nayavnist elektroniv v g orbitalyah yaki ne isnuyut v konfiguraciyi elektronnih orbitalej bud yakogo vidomogo u danij chas elementa povinno dozvoliti nevidomim gibridnim orbitalyam formuvati i vplivati na himiyu superaktinoyidiv novimi sposobami hocha vidsutnist g elektroniv u vidomih elementah robit prognozuvannya himiyi supekaktinoyida bilsh skladnimi Superaktinoyidi 121Ubu 122Ubb 123Ubt 124Ubq 125Ubp 126Ubh 127Ubs 128Ubo 129Ube 130Utn 131Utu 132Utb 133Utt 134Utq 135Utp 136Uth137Uts 138Uto 139Ute 140Uqn 141Uqu 142Uqb 143Uqt 144Uqq 145Uqp 146Uqh 147Uqs 148Uqo 149Uqe 150Upn 151Upu 152UpbDzherela RedaguvatiB Fricke W Greiner amp J T Waber Superheavy elements A prediction of their chemical and physical properties Arhivovano 4 zhovtnya 2013 u Wayback Machine Theoretica chimica acta volume 21 s 235 260 1971 Burkhard Fricke Superheavy elements a prediction of their chemical and physical properties Arhivovano 19 kvitnya 2020 u Wayback Machine Recent Impact of Physics on Inorganic Chemistry 2007 s 89 144 DOI 10 1007 BFb0116498 ISBN 978 3 540 37395 7 nbsp Ce nezavershena stattya z himiyi Vi mozhete dopomogti proyektu vipravivshi abo dopisavshi yiyi Otrimano z https uk wikipedia org w index php title Superaktinoyidi amp oldid 38437749