Are there General Circulation Models that can simulate the atmosphere of Venus? I would like to know what would happen with the atmosphere of Venus when it gets tidally locked, i.e. when one side would perpetually face the Sun.
Probably a thermal low would be at the subsolar region then.

At the surface Venus has an atmospheric pressure of 92 atm. and a temperature of 462$⁰$ C.

Are there General Circulation Models or Global Climate Models that can handle such input parameters ?

If so, are there GCM users (groups, universities etc.) who could run a tidally locked Venus simulation ?
I'm not sure of their current status, but I read some papers based on these models a few years ago:


Oxford Planetary Unified Model System for Venus (OPUS-V), which is based on an old version of the UK Met Office climate model, HadCM3 (paper from 2016).
ROCKE-3D at Nasa GISS, which is based on an old version of the GISS ModelE2‐R climate model (blog article and paper from 2016).


It looks like the introduction of Yamamoto et al (2019) has a more up-to-date summary of the current set of models, and there's quite a healthy selection from groups around the world.