Zengxiu Zhao

Oct 1, 2024 | nature.com | Bo Chen |Han Wang |Kaiguo Chen |Xiaoxiang Yu |Yong Hou |Zengxiu Zhao | +3 more

AbstractThe immiscibility of hydrogen-helium mixture under the temperature and pressure conditions of planetary interiors is crucial for understanding the structures of gas giant planets (e.g., Jupiter and Saturn). While the experimental probe at such extreme conditions is challenging, theoretical simulation is heavily relied in an effort to unravel the mixing behavior of hydrogen and helium.