2020
DOI: 10.1016/j.lithos.2020.105614
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Melting of the juvenile lower crust in a far-field response to roll-back of the southern Neotethyan oceanic lithosphere: the Oligocene adakitic dacites, NE Turkey

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Cited by 10 publications
(7 citation statements)
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“…The XSG porphyritic granite samples plot between the depletedmantle and chondrite Hf isotopic lines with εHf(t) values of +2.4 − +4.6 (Figure 9a,b), indicating that the XSG porphyritic granite formed from magmas derived from a juvenile lower crust source (Karsli et al, 2020;Wang, Zheng, & Zhu, 2019;Zhou, Lü, & Wang, 2011). These samples also have T DM2 ages of 1,123-981 Ma, suggesting that their juvenile lower crustal source formed during the Mesoproterozoic-Neoproterozoic period.…”
Section: Middle Triassic Granitoidsmentioning
confidence: 98%
“…The XSG porphyritic granite samples plot between the depletedmantle and chondrite Hf isotopic lines with εHf(t) values of +2.4 − +4.6 (Figure 9a,b), indicating that the XSG porphyritic granite formed from magmas derived from a juvenile lower crust source (Karsli et al, 2020;Wang, Zheng, & Zhu, 2019;Zhou, Lü, & Wang, 2011). These samples also have T DM2 ages of 1,123-981 Ma, suggesting that their juvenile lower crustal source formed during the Mesoproterozoic-Neoproterozoic period.…”
Section: Middle Triassic Granitoidsmentioning
confidence: 98%
“…In such a scenario, the Meiji dacites might be products of magmas derived from the lower continental crust beneath the SCB. Modeling using whole Sm/Yb and La/Yb ratios (Karsli et al, 2020) suggests that the Meiji dacites can be produced by <40% partial melting of amphibolites containing ∼10% garnet in the lower continental crust (Figure 12A, B). On the other hand, the Meiji dacites are compositionally different from adakites produced by partial melting of a subducted slab (Defant and Drummond, 1990) or thickened lower crust (Ma et al, 2016).…”
Section: Petrogenesis Of the Meiji Atoll Dacitesmentioning
confidence: 99%
“…Subduction of the southern Neotethys branch and subsequent Arabia-Eurasia collision and post-collision evolution generated Cenozoic magmatism in the Iranian Urumieh-Dokhtar (Chiu et al, 2013;Omrani et al, 2008) and Alborz magmatic arcs (Aghazadeh et al, 2011(Aghazadeh et al, , 2010Asiabanha and Foden, 2012;Castro et al, 2013;Verdel et al, 2011;Vincent et al, 2005), the SAB (Moritz et al, 2016b;Rezeau et al, 2018Rezeau et al, , 2017Rezeau et al, , 2016Sahakyan et al, 2016), the Eastern Pontides (Aydınçakır and S ¸en, 2013;Dokuz et al, 2019;Eyuboglu et al, 2017;Karsli et al, 2020bKarsli et al, , 2020aKarsli et al, , 2019Karsli et al, , 2011Kaygusuz and Öztürk, 2015) and the TAP ( ˙Imer et al, 2013;Keskin, 2003;Rabayrol et al, 2019;Schleiffarth et al, 2018).…”
Section: Geological Setting and Geodynamic Evolution Of The South Arm...mentioning
confidence: 99%