Rutherford’un \u00f6\u011frencileri Geiger ve Marsden, alfa kayna\u011f\u0131n\u0131, \u00fczerinde k\u00fc\u00e7\u00fck bir delik bulunan kur\u015fun perdenin arkas\u0131na yerle\u015ftirdiler. B\u00f6ylelikle hedefi k\u00fc\u00e7\u00fcltmek ve ince bir alfa par\u00e7ac\u0131klar\u0131 demeti elde etmek ama\u00e7lanm\u0131\u015ft\u0131. Alt\u0131n yapra\u011f\u0131n \u00f6b\u00fcr yan\u0131na, kendisine alfa par\u00e7ac\u0131\u011f\u0131 \u00e7arpt\u0131\u011f\u0131 zaman g\u00f6r\u00fcn\u00fcr \u0131\u015f\u0131k par\u0131lt\u0131s\u0131 veren, hareketli, \u00e7inko s\u00fclf\u00fcrl\u00fc ekran yerle\u015ftirilmi\u015fti.<\/p>\n
Beklenen \u015fey, alfa par\u00e7ac\u0131klar\u0131n\u0131n \u00e7o\u011funun yaprak i\u00e7inden do\u011frudan ge\u00e7ece\u011fi, belki baz\u0131lar\u0131n\u0131n \u00e7ok k\u00fc\u00e7\u00fck sapmalara u\u011frayaca\u011f\u0131yd\u0131. Bu beklenti, Thomson Atom Modeli’nin sonucudur. \u00c7\u00fcnk\u00fc Thomson Atom Modeli do\u011fruysa, ince metal levhadan ge\u00e7en alfa par\u00e7ac\u0131klar\u0131 \u00fczerine yaln\u0131zca zay\u0131f elektriksel kuvvetler etkir ve alfa par\u00e7ac\u0131klar\u0131n\u0131n momentumlar\u0131, bunlar\u0131n ilk yollar\u0131ndan \u00e7ok k\u00fc\u00e7\u00fck sapmalar olacak \u015fekilde ilerlemelerini sa\u011flar.<\/p>\n
Geiger ve Marsden, alfa par\u00e7ac\u0131klar\u0131n\u0131n \u00e7o\u011funun sapmadan ilerledi\u011fini, baz\u0131lar\u0131n\u0131n \u00e7ok geni\u015f a\u00e7\u0131larda sa\u00e7\u0131ld\u0131\u011f\u0131n\u0131, hatta \u00e7ok az bir k\u0131sm\u0131n\u0131n gerisin geriye d\u00f6nd\u00fc\u011f\u00fcn\u00fc g\u00f6rd\u00fcler. Geli\u015f do\u011frultusuyla 180 derece a\u00e7\u0131 yapacak \u015fekilde geri sa\u00e7\u0131lan bu par\u00e7ac\u0131klar, direkt olarak bir \u00e7ekirde\u011fe y\u00f6nelir ve kafa kafaya \u00e7arp\u0131\u015fma olur.<\/p>\n
Bu modelde, pozitif y\u00fckl\u00fc alfa par\u00e7ac\u0131klar\u0131yla atomdaki elektronlar\u0131n ili\u015fkisi merak edilir. Elektronlar pek k\u00fc\u00e7\u00fck k\u00fctleli oldu\u011fu i\u00e7in alfa par\u00e7ac\u0131klar\u0131n\u0131n hareketinde \u00f6nemli bir etkide bulunmaz.<\/p>\n
Alfa par\u00e7ac\u0131klar\u0131, elektronlardan 7.000 defa daha a\u011f\u0131r k\u00fctleli par\u00e7ac\u0131klard\u0131. \u00dcstelik bu deneyde kullan\u0131lan alfa par\u00e7ac\u0131klar\u0131n\u0131n h\u0131z\u0131 y\u00fcksekti. Alfa par\u00e7ac\u0131klar\u0131n\u0131 bu derece sapt\u0131rabilmek i\u00e7in b\u00fcy\u00fck kuvvetler uygulanmas\u0131 gerekti\u011fi a\u00e7\u0131kt\u0131. Bu kuvvetlerin Thomson Atom Modeli’ndeki elektriksel kuvvetlere g\u00f6re 100 milyon kat g\u00fc\u00e7l\u00fc oldu\u011fu hesaplan\u0131yordu.<\/p>\n
Rutherford, sonu\u00e7lar\u0131 a\u00e7\u0131klamak i\u00e7in, bir atomun pozitif y\u00fckl\u00fc bir \u00e7ekirdek ile biraz uzaktaki elektronlardan olu\u015ftu\u011funu \u00f6nerdi. Buna g\u00f6re atomun pozitif y\u00fck\u00fc ve k\u00fctlesi atom \u00e7ekirde\u011finde toplanm\u0131\u015ft\u0131.<\/p>\n
Geiger ve Marsden’in deneyleri, daha sonraki benzer \u00e7al\u0131\u015fmalar, hedefleri olu\u015fturan de\u011fi\u015fik metallerin \u00e7ekirdekleri hakk\u0131nda bilgiler verdi. Bir alfa par\u00e7ac\u0131\u011f\u0131n\u0131n, bir \u00e7ekirdek yak\u0131n\u0131ndan ge\u00e7erken u\u011frad\u0131\u011f\u0131 sapma (kar\u015f\u0131la\u015ft\u0131\u011f\u0131 elektriksel alan), \u00e7ekirdek y\u00fck\u00fcn\u00fcn b\u00fcy\u00fckl\u00fc\u011f\u00fcne ba\u011fl\u0131d\u0131r. Bu sapmalardan yanrarlan\u0131larak \u00e7ekirdek y\u00fck\u00fc ve \u00e7ekirdek boyutu konusunda bilgiler elde edildi.<\/p>\n
\u00c7ekirdek kuvvetleri \u00e7ok k\u0131sa mesafeli kuvvetlerdi. Atom \u00e7ekirde\u011fiyle ilgili kilometre ta\u015f\u0131 say\u0131lan di\u011fer olaylar \u015funlard\u0131r:<\/p>\n
1930 y\u0131l\u0131nda Cockroft ve Walton h\u0131zland\u0131r\u0131lm\u0131\u015f par\u00e7ac\u0131klar\u0131n kullan\u0131lmas\u0131yla ger\u00e7ekle\u015ftirlen \u00e7ekirdek tepkimelerinin g\u00f6zlenmesi<\/p>\n
1932 y\u0131l\u0131nda Chadwick’in n\u00f6tronu bulmas\u0131<\/p>\n
1933 y\u0131l\u0131nda Joliot ve \u0130rene Curie’nin yapay radyoaktifli\u011fi bulmas\u0131<\/p>\n
1938’de Hahn ve Strassman’\u0131n \u00e7ekirdek b\u00f6l\u00fcnmesini (\u00e7ekirdek fisyonunu) bulmas\u0131<\/p>\n
1942 y\u0131l\u0131nda Fermi ve ekibinin kontrol edilebilen ilk fisyon reakt\u00f6r\u00fcn\u00fcn geli\u015ftirilmesi<\/p>\n
Rutherford\u2019un sa\u00e7\u0131lma deneyleri ilgi \u00e7ekici idiyse de, klasik fizik a\u00e7\u0131s\u0131ndan onun gezegensel resmi san\u0131ld\u0131\u011f\u0131 kadar dengeli de\u011fildi. Doyurucu olmayan durum k\u0131sa s\u00fcrede de\u011fi\u015fti. 1912 c\u0131var\u0131nda Rutherford, Manchester\u2019dan arkada\u015f\u0131 Boltwood\u2019a \u015f\u00f6yle yaz\u0131yordu: “Bir Danimarkal\u0131 olan Bohr, Cambridge\u2019den \u00e7\u0131km\u0131\u015f, radyoaktif \u00e7al\u0131\u015fmada baz\u0131 deneyler yapmak \u00fczere buraya geliyor”.<\/p>\n
Cambridge\u2019de, J.J. Thomson\u2019un bir \u00f6\u011frenci olan Niels Bohr, kendi memleketine, Kopenhag\u2019a d\u00f6nmeden \u00f6nce, Manchester\u2019da yar\u0131m y\u0131ldan az bir s\u00fcre kald\u0131. Ancak, k\u0131sa ziyaretine ra\u011fmen, Rutherford gen\u00e7 Danimarkal\u0131 \u00fczerinde etkili oldu.<\/p>\n
Bohr’un ilgisini \u00e7ekmi\u015f olan atomik yap\u0131 problemi, yarat\u0131c\u0131 cesaretli bir ad\u0131m att\u0131: Klasik fizi\u011fin baz\u0131 kurallar\u0131n\u0131 b\u0131rakt\u0131 ve onun yerine atomik yap\u0131 problemine Planck\u2019\u0131n ve Einstein\u2019in Kuantum Kuram\u0131’n\u0131 uygulad\u0131. Dikkate de\u011ferdir ki o zamanlar bilinen Kuantum Kuram\u0131’n\u0131n birka\u00e7 \u00f6zelli\u011fi problemi \u00e7\u00f6zebilirdi (Klasik fizikle \u00e7eli\u015fki konusuna ald\u0131r\u0131\u015f edilmedi\u011fi s\u00fcrece).<\/p>\n
Bohr, basit\u00e7e, \u00e7ekirdek etraf\u0131ndaki y\u00f6r\u00fcngelerdeki elektronlar\u0131n \u0131\u015f\u0131k yaymad\u0131klar\u0131n\u0131 ve atomlar\u0131n yayd\u0131\u011f\u0131 \u0131\u015f\u0131\u011f\u0131n bir ba\u015fka fiziksel yap\u0131n\u0131n sonucu oldu\u011funu varsayd\u0131. Bohr, Planck\u2019\u0131n enerjinin kuantla\u015fmas\u0131 fikrinin, elekronlar i\u00e7in ancak belli y\u00f6r\u00fcngelerin m\u00fcmk\u00fcn oldu\u011fu anlam\u0131na geldi\u011fini g\u00f6sterdi. Atomlar\u0131n kararl\u0131l\u0131\u011f\u0131n\u0131 korumak i\u00e7in Bohr, y\u00f6r\u00fcngedeki elektronun onun alt\u0131na d\u00fc\u015femeyece\u011fi en d\u00fc\u015f\u00fck enerjili y\u00f6r\u00fcnge konusunda bir \u00f6nermede bulundu.<\/p>\n
Bir elektron daha y\u00fcksek bir y\u00f6r\u00fcngeden, daha al\u00e7a\u011f\u0131na d\u00fc\u015ferken, b\u00f6ylece enerji kaybederken, bu elektronu ta\u015f\u0131yan atom \u0131\u015f\u0131k yayar, bu da kaybedilen enerjiyi ta\u015f\u0131r. Yaln\u0131zca belli elektron y\u00f6r\u00fcngelerine izin verildi\u011fi i\u00e7in, elektronlar\u0131n y\u00f6r\u00fcngeler aras\u0131nda yaln\u0131z belli s\u0131\u00e7ramalar olabilir ve sonu\u00e7 olarak, yay\u0131lan \u0131\u015f\u0131\u011f\u0131n enerjisi kuantla\u015f\u0131r (Nicelik olarak ifade edilebilir).<\/p>\n
I\u015f\u0131\u011f\u0131n enerjisi, rengi ile ba\u011flant\u0131l\u0131 oldu\u011fu i\u00e7in, atomlar taraf\u0131ndan ancak belli renklerde \u0131\u015f\u0131k yay\u0131labilir. Bu \u015fekilde Bohr\u2019un teorik Atom Modeli, gizemli tayf \u00e7izgilerinin varl\u0131\u011f\u0131n\u0131 a\u00e7\u0131klamaktad\u0131r. Her farkl\u0131 atomun tek ve belli renklerde \u0131\u015f\u0131k yayd\u0131\u011f\u0131n\u0131 ifade eden deneysel olarak g\u00f6zlemlenmi\u015f ger\u00e7ek, atomlar\u0131n kuantum yap\u0131s\u0131n\u0131 a\u00e7\u0131\u011fa \u00e7\u0131karm\u0131\u015ft\u0131r.<\/p>\n
Bohr\u2019un atomunun enerji d\u00fczeylerini imgelemenin bir yolu, harp gibi, yayl\u0131 bir m\u00fczik enst\u00fcrman\u0131 d\u00fc\u015f\u00fcnmektir. \u00c7al\u0131nd\u0131\u011f\u0131 zaman her yaydan belli bir titre\u015fim veya ses \u00e7\u0131kar. Benzer \u015fekilde bir elektron, atomdaki y\u00f6r\u00fcngelerde atlarken, belli bir titre\u015fimi veya rengi olan \u0131\u015f\u0131k yay\u0131lmas\u0131 olur. Bu da kesintili \u0131\u015f\u0131k tayf\u0131n\u0131n kayna\u011f\u0131d\u0131r.<\/p>\n
Bohr yeni fikirlerini, tek bir protonla onun \u00e7evresinde y\u00f6r\u00fcngede tek bir elektronu olan en basit atoma, hidrojene uygulad\u0131. B\u00f6yle basit bir atom incelemenin avantaj\u0131, elektronun izin verilen y\u00f6r\u00fcngelerinin kesin olarak hesaplanabilir olmas\u0131 ve bu nedenle de hidrojenden \u00e7\u0131kan \u0131\u015f\u0131k tayf\u0131n\u0131n belirlenebilmesidir.<\/p>\n
Bohr\u2019un kendi teorik Atom Modeli’ne dayanan hidrojen \u0131\u015f\u0131k tayf\u0131 ile ilgili hesaplar\u0131, deneysel olarak g\u00f6zlemlenmi\u015f olan tayfa yeterince uygun sonu\u00e7 verdi. Teori ile deney aras\u0131nda b\u00f6yle uyum rasgele olamazd\u0131. Bu durum, Bohr\u2019un, Kuantum Teorisi’nden ald\u0131\u011f\u0131 fikirler bile\u015fiminin do\u011fru \u00e7\u0131kt\u0131\u011f\u0131 anlam\u0131na geliyordu.<\/p>\n
Kuramsal fizik\u00e7iler, Bohr\u2019un fikirlerini ald\u0131lar ve daha karma\u015f\u0131k atomlara uygulad\u0131lar. Ancak, her b\u00fcy\u00fck bilimsel ilerleme gibi, Bohr\u2019un modeli pek \u00e7ok yeni soruya (Daha \u00f6nce sorulamayan sorulara) yol a\u00e7t\u0131. Bir elektron ne zaman y\u00f6r\u00fcngesini de\u011fi\u015ftirip atomdan \u0131\u015f\u0131k yay\u0131lmas\u0131na yol a\u00e7ar? Yay\u0131lan \u0131\u015f\u0131k hangi do\u011frultuda ilerler ve neden?<\/p>\n
Bu sorular Einstein\u2019\u0131 zorlad\u0131. Klasik fizi\u011fe g\u00f6re, hareketin yasalar\u0131 atom gibi bir fiziksel sistemin gelecekteki davran\u0131\u015f\u0131n\u0131 kesin olarak belirler. Fakat \u0131\u015f\u0131k yayan atomlar ani ve \u00f6nceden belirlenmemi\u015f \u015fekilde hareket ediyor g\u00f6r\u00fcn\u00fcyorlard\u0131. Atomlar s\u0131\u00e7r\u0131yor. Fakat neden ve hangi y\u00f6nde? Einstein, ayn\u0131 anili\u011fin radyoaktivitenin de \u00f6zelli\u011fi oldu\u011funu kavrad\u0131.<\/p>\n
Ba\u015flang\u0131\u00e7ta fizik\u00e7iler, atomlar\u0131n davran\u0131\u015f\u0131n\u0131 klas\u0131k elektromanyetizm teorisi \u00e7er\u00e7evesine uydurmaya \u00e7al\u0131\u015ft\u0131lar ve \u0131\u015f\u0131k kuantas\u0131 kullanmadan, kuantum s\u0131\u00e7ramalar\u0131 bilmecesini yan\u0131tlamak i\u00e7in umutsuz giri\u015fimlerde bulundular. 1924’te Niels Bohr, Hendrik Kramers ve John Slater, atom d\u00fczeyinde enerji ve momentumun korunumu yasalar\u0131n\u0131 terketme pahas\u0131na bu yakla\u015f\u0131m\u0131 savunan bir yaz\u0131 yazd\u0131lar.<\/p>\n
Bu devrimci bir \u00f6neriydi. \u00c7\u00fcnk\u00fc bu yasalar en iyi test edilmi\u015f fizik yasalar aas\u0131nda bunuyorlard\u0131. Bu \u00f6nerini yap\u0131ld\u0131\u011f\u0131 zamanda, korunum (sak\u0131n\u0131m) yasalar\u0131n\u0131 tek tek atomik s\u00fcre\u00e7ler i\u00e7in ge\u00e7erli oldu\u011funu g\u00f6steren hi\u00e7bir do\u011frudan deneysel kan\u0131 olmam\u0131\u015ft\u0131. Ancak bu k\u0131sa s\u00fcrede ger\u00e7ekle\u015fti.<\/p>\n
Arthur H. Compton ve A. W. Simon, elektronlardan tek tek fotonlar, \u0131\u015f\u0131k par\u00e7ac\u0131klar\u0131 sa\u00e7\u0131lmas\u0131n\u0131 sa\u011flad\u0131lar. Tek tek elektronlar\u0131n izlerini g\u00f6r\u00fcnt\u00fcleyen bir cihaz olan Wilson Bulut B\u00f6lmesi kullanarak, y\u00fcksek hassasl\u0131k derecesi ile tek tek atomik s\u00fcre\u00e7ler i\u00e7in korunum yasalar\u0131n\u0131 do\u011frulad\u0131lar. Fizik\u00e7ilerin \u00e7o\u011fu i\u00e7in 1925’te yap\u0131lan bu deneyler, Einstein\u2019\u0131n 1905 y\u0131l\u0131ndaki \u0131\u015f\u0131k kuantumu \u00f6nerisini destekledi.<\/p>\n
Rutherford ve Compton\u2019ununkiler gibi \u00e7ok say\u0131da yeni atomik deneyle, atomun yap\u0131s\u0131 a\u00e7a\u011fa \u00e7\u0131kar\u0131lm\u0131\u015ft\u0131. Bu deneyler, teorik fizik\u00e7ileri yeni ve bilinmeyen bir d\u00fcnyaya ge\u00e7meye zorlad\u0131; al\u0131\u015f\u0131lm\u0131\u015f olar klasik fizi\u011fin yasalar\u0131 art\u0131k i\u015flemiyor g\u00f6r\u00fcn\u00fcyordu. Atomda insan zihni yeni bir mesaj\u0131 alm\u0131\u015ft\u0131. Atomik mikrod\u00fcnyan\u0131n yap\u0131s\u0131nda yeni bir fizik a\u00e7\u0131\u011fa \u00e7\u0131kt\u0131. Y\u00fczy\u0131llarca deney ve fiziksel teorilerle desteklenen determinizmin d\u00fcnya g\u00f6r\u00fc\u015f\u00fc y\u0131k\u0131lmak \u00fczereydi.<\/p>\n
Bohr, Compton ve Simon\u2019un deneylerinin sonu\u00e7lar\u0131n\u0131n, hem Korunum Yasalar\u0131n\u0131n do\u011frulu\u011fu, hem des I\u015f\u0131k Kuantumu veya fotonun varl\u0131\u011f\u0131 anlam\u0131na geldi\u011fini kabul etti. Temmuz 1925’te \u015fu sonucu \u00f6zetledi: “Klasik elektrodinamik teorinin gerekli genelle\u015fmesinin, do\u011fan\u0131n tan\u0131m\u0131n\u0131 bu g\u00fcne kadar \u00fczerine kurulmu\u015f oldu\u011fu kavramlarda k\u00f6kl\u00fc bir devrimi gerektirdi\u011fi ger\u00e7e\u011fine haz\u0131r olunmal\u0131d\u0131r.” Bohr bu devrime haz\u0131rd\u0131. Bu, k\u0131sa s\u00fcrede ger\u00e7ekle\u015fti. Bunun ilk ad\u0131m\u0131 halihaz\u0131rda, kuzey denizinde bir k\u00fc\u00e7\u00fck adada at\u0131lm\u0131\u015ft\u0131.”<\/p>\n
Sa\u00e7\u0131c\u0131 metal yapraktan, floresans ekrana gelen alfa par\u00e7ac\u0131klar\u0131n\u0131n, birim y\u00fczeye d\u00fc\u015fen say\u0131s\u0131, metal yapra\u011f\u0131n kal\u0131nl\u0131\u011f\u0131yla, metal yaprakta birim hacimdeki atom say\u0131s\u0131yla ve atomdaki \u00e7ekirdek y\u00fck\u00fcn\u00fcn karesiyle do\u011fru orant\u0131l\u0131d\u0131r. Deneyler pek \u00e7ok \u00e7ekirde\u011fin yakla\u015f\u0131k k\u00fcresel geometriye sahip olduklar\u0131 ve t\u00fcm \u00e7ekirdeklerin yakla\u015f\u0131k ayn\u0131 yo\u011funlu\u011fa sahip oldu\u011funu g\u00f6sterdi.<\/p>\n
Thomson, kendi atom modelinde, elektronlar\u0131n pozitif madde i\u00e7inde g\u00f6m\u00fcl\u00fc ve bu nedenle de hareket edemez oldu\u011funu tasarlam\u0131\u015ft\u0131. Rutherford Modeli’nde elektronlar durgun olamaz. Elektronlar, elektrostatik \u00e7ekim sonucu spiral bir hareketle \u00e7ekirde\u011fe d\u00fc\u015fecektir (klasik fizik yasalar\u0131na g\u00f6re). Oysa atomla,r yads\u0131namaz kararl\u0131l\u0131klar\u0131yla ortadad\u0131r.<\/p>\n
Rutherford modeli \u015fu iki soruyu yan\u0131tlayam\u0131yordu:<\/p>\n
Elektronlar, \u00e7ekirdek \u00fczerine d\u00fc\u015fmeden nas\u0131l hareket ediyor?<\/p>\n
\u00c7ekirdek boyutu, on \u00fczeri eksi ond\u00f6rt metre ve daha k\u00fc\u00e7\u00fck boyutlarda oldu\u011fu halde pozitif y\u00fck, bu k\u00fc\u00e7\u00fck ve yo\u011fun hacimde nas\u0131l da\u011f\u0131lmadan durabiliyordu?<\/p>\n","protected":false},"excerpt":{"rendered":"
Rutherford’un \u00f6\u011frencileri Geiger ve Marsden, alfa kayna\u011f\u0131n\u0131, \u00fczerinde k\u00fc\u00e7\u00fck bir delik bulunan kur\u015fun perdenin arkas\u0131na yerle\u015ftirdiler. B\u00f6ylelikle hedefi k\u00fc\u00e7\u00fcltmek ve ince bir alfa par\u00e7ac\u0131klar\u0131 demeti elde etmek ama\u00e7lanm\u0131\u015ft\u0131. Alt\u0131n yapra\u011f\u0131n \u00f6b\u00fcr yan\u0131na, kendisine alfa par\u00e7ac\u0131\u011f\u0131 \u00e7arpt\u0131\u011f\u0131 zaman g\u00f6r\u00fcn\u00fcr \u0131\u015f\u0131k par\u0131lt\u0131s\u0131 veren, hareketli, \u00e7inko s\u00fclf\u00fcrl\u00fc ekran yerle\u015ftirilmi\u015fti. Beklenen \u015fey, alfa par\u00e7ac\u0131klar\u0131n\u0131n \u00e7o\u011funun yaprak i\u00e7inden do\u011frudan ge\u00e7ece\u011fi, …<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[1407,1403],"tags":[5147,2722,2134,6865,6864,2758,6863,5007],"class_list":["post-2807","post","type-post","status-publish","format-standard","hentry","category-fen-ve-teknoloji-odevleri","category-odevler","tag-bohr","tag-einstein","tag-elektron","tag-klasik-fizik-yasalari","tag-momentum","tag-radyoaktif","tag-rutherfordun-atom-modeli","tag-thomson-atom-modeli"],"_links":{"self":[{"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/posts\/2807","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/comments?post=2807"}],"version-history":[{"count":0,"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/posts\/2807\/revisions"}],"wp:attachment":[{"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/media?parent=2807"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/categories?post=2807"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.islamidavet.com\/kutuphane\/wp-json\/wp\/v2\/tags?post=2807"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}