{"id":4383,"date":"2019-03-16T19:57:57","date_gmt":"2019-03-16T16:57:57","guid":{"rendered":"https:\/\/www.berjournal.com\/?p=4383"},"modified":"2019-03-23T02:37:25","modified_gmt":"2019-03-22T23:37:25","slug":"star-models-an-application-for-gdp-per-capita-growth-rate","status":"publish","type":"post","link":"https:\/\/www.berjournal.com\/tr\/star-models-an-application-for-gdp-per-capita-growth-rate","title":{"rendered":"STAR Modelleri: Ki\u015fi Ba\u015f\u0131na GSY\u0130H B\u00fcy\u00fcme H\u0131z\u0131 \u0130\u00e7in Bir Uygulama"},"content":{"rendered":"

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Makale Bilgileri<\/td>\n<\/tr>\n
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Dergi:<\/td>\nBusiness and Economics Research Journal<\/td>\n<\/tr>\n
Makalenin Ba\u015fl\u0131\u011f\u0131:<\/td>\nSTAR Modelleri: Ki\u015fi Ba\u015f\u0131na GSY\u0130H B\u00fcy\u00fcme H\u0131z\u0131 \u0130\u00e7in Bir Uygulama<\/td>\n<\/tr>\n
Yazar(lar):<\/td>\nFatma Idil Baktemur<\/td>\n<\/tr>\n
Cilt:<\/td>\n10<\/td>\n<\/tr>\n
Say\u0131:<\/td>\n2<\/td>\n<\/tr>\n
Y\u0131l:<\/td>\n2019<\/td>\n<\/tr>\n
Sayfa:<\/td>\n405-414<\/td>\n<\/tr>\n
ISSN:<\/td>\n2619-9491<\/td>\n<\/tr>\n
DOI Numaras\u0131:<\/td>\n10.20409\/berj.2019.176<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<\/td>\n<\/tr>\n
\u00d6z<\/td>\n<\/tr>\n
Do\u011frusall\u0131k varsay\u0131m\u0131 uzun s\u00fcre ge\u00e7erli olmu\u015ftur ancak iktisadi zaman serilerinin \u00e7o\u011fu asimetrik davran\u0131\u015flar sergilemektedir. Hesaplama g\u00fc\u00e7l\u00fcklerinin kald\u0131r\u0131lmas\u0131yla uygulamada do\u011frusal olmayan zaman serileri \u00e7al\u0131\u015fmalar\u0131n\u0131n say\u0131s\u0131 artm\u0131\u015ft\u0131r. Markov rejim de\u011fi\u015fim modelleri, TAR ve STAR modelleri do\u011frusal olmayan zaman serileri \u00e7al\u0131\u015fmalar\u0131na \u00f6rnek verilebilir. Ki\u015fi ba\u015f\u0131na GSY\u0130H, iktisadi b\u00fcy\u00fcmenin \u00f6nemli bir unsurudur ve pek \u00e7ok \u00e7al\u0131\u015fmaya konu olmu\u015ftur. 1961-2017 y\u0131ll\u0131k verilerini kapsayan bu \u00e7al\u0131\u015fma T\u00fcrkiye i\u00e7in ki\u015fi ba\u015f\u0131na GSY\u0130H b\u00fcy\u00fcme h\u0131z\u0131n\u0131n do\u011frusal olmayan yap\u0131s\u0131n\u0131 STAR modelleri ile incelemi\u015ftir. Seri birim k\u00f6k testi sonu\u00e7lar\u0131na g\u00f6re dura\u011fand\u0131r ve modelin gecikme uzunlu\u011fu iki olarak bulunmu\u015ftur. Ba\u011f\u0131ml\u0131 de\u011fi\u015fkenin gecikmelerine g\u00f6re tek tek ge\u00e7i\u015f de\u011fi\u015fkenleri olu\u015fturulmu\u015f ve modelin do\u011frusall\u0131\u011f\u0131 do\u011frusal olmama alternatifine g\u00f6re test edilmi\u015ftir. Birinci gecikme ge\u00e7i\u015f de\u011fi\u015fkeni olarak se\u00e7ilmi\u015ftir. %5 anlaml\u0131l\u0131k d\u00fczeyinde do\u011frusall\u0131k hipotezi reddedilmi\u015ftir. \u00c7al\u0131\u015fman\u0131n bulgular\u0131 b\u00fcy\u00fcme i\u00e7in LSTAR tipi modellemenin uygun oldu\u011funu g\u00f6stermektedir. Uygun model LSTAR oldu\u011fu i\u00e7in ge\u00e7i\u015f de\u011fi\u015fkeni standart hatas\u0131na b\u00f6l\u00fcnerek standartla\u015ft\u0131r\u0131lm\u0131\u015ft\u0131r. Ge\u00e7i\u015f yumu\u015fakl\u0131\u011f\u0131n\u0131 g\u00f6steren parametre bir rejimden di\u011fer rejime ge\u00e7i\u015fin h\u0131zl\u0131 oldu\u011funu g\u00f6stermektedir.<\/td>\n<\/tr>\n
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Anahtar Kelimeler:<\/td>\nDo\u011frusal Olmama, GSY\u0130H, B\u00fcy\u00fcme, STAR Modelleri, Rejim Ge\u00e7i\u015fi<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<\/td>\n<\/tr>\n
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JEL S\u0131n\u0131fland\u0131rmas\u0131:<\/td>\nC24, C01, C22<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n
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Makale Bilgileri Dergi: Business and Economics Research Journal Makalenin Ba\u015fl\u0131\u011f\u0131: STAR Modelleri: Ki\u015fi Ba\u015f\u0131na GSY\u0130H B\u00fcy\u00fcme H\u0131z\u0131 \u0130\u00e7in Bir Uygulama Yazar(lar): Fatma Idil Baktemur Cilt: 10 Say\u0131: 2 Y\u0131l: 2019 Sayfa: 405-414 ISSN: 2619-9491 DOI Numaras\u0131: 10.20409\/berj.2019.176 \u00d6z Do\u011frusall\u0131k varsay\u0131m\u0131 uzun s\u00fcre ge\u00e7erli olmu\u015ftur ancak iktisadi zaman serilerinin \u00e7o\u011fu asimetrik davran\u0131\u015flar sergilemektedir. Hesaplama g\u00fc\u00e7l\u00fcklerinin kald\u0131r\u0131lmas\u0131yla […]<\/p>\n

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