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the formation and evolution of magma oceans in planets. By recreating the extreme conditions present during the early stages of planetary accretion, the project aims to elucidate the physical and chemical
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application. In this PhD, the focus is to rationally develop and process highly crystalline, X-ray sensitive lead-free perovskite material layers through micromanaging their electronic structure by composition
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. Application Deadline: May 27th 2024 Selection Deadline: June 17th 2024 Eligibility criteria Applicants with a Master degree or an equivalent in astrophysics or physics are eligible for the position. High
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mindset You have an excellent proficiency in the English language (both speaking and writing) Selection process Interested applicants should submit:- a motivation letter with a statement of skills and
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communication skills Fluid in English Selection process For more information please contact Prof. dr. Lies Langouche, tel.: +32 16 33 05 24, mail: [email protected] or Prof. dr. Greet Van den Berghe
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plus.- Candidates should be able to work independently and possess a critical mindset. Selection process For more information or questions about these positions and potential fit, please contact Prof
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master's degree in Physics or Astronomy or Psychology or Educational Sciences - with very good study results (at least level 'cum laude'), or will obtain this very soon a teacher's degree from a university
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vector-autoregressive modeling is an asset. Selection process For more information please contact Prof. dr. Kim De Roover, mail: [email protected] . Applications should consist of a motivation
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stability, and hinder their large-scale device application. In this PhD, the focus is to rationally develop and process highly crystalline, X-ray sensitive lead-free perovskite materials through micromanaging
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characteristics to succeed in this endeavour. This PhD position will be supervised by Prof. Nicolas Bastardoz and co-supervised by Prof. Anneleen Forrier Selection process For more information please contact Prof