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On Apr 19, 2023, at 1:21 AM, Kang, SiYoon <rkd52...@gmail.com> wrote:
Oh sorry. DeCaluwe.
i think i misrepresented it.What i was saying was that i was curious about the reference equations of how to calculate Cp from real-gas EOS (RK or PR) in the source file (c++).as far as i know, Cp should be dHdT_P because it represents specific heat under constant pressure.but in the source file, dHdT_V appears to represent Cp under constant volume conditions.
<dHdT_V.png>
i woud appreciate it if you could check it again.Thank you2023년 4월 19일 수요일 오후 3시 50분 12초 UTC+9에 S. DeCaluwe님이 작성:Hi Simon,It is not all that clear what you are referring to. Do you feel that the algorithm in the code should look different?We have the derivations in a document somewhere (getting these onto the website is currently on the to-do list), but in the mean time I’ll just point out that the algorithms are tested against a finite-difference approximation for dh/dT at constant P, here.Best regards,StevenOn Apr 19, 2023, at 12:03 AM, Kang, SiYoon <rkd52...@gmail.com> wrote:Hi, everyone.Now I'm studying real-gas eos.but i have a question about Peng-robinson and Redlich-Kwong EOS.i've seen a different way of calculating Cp at constant pressure.but the Cantera calculated the Cp at constant volume.so I wonder where it came from.Thank you !--
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<dHdT_V.png>