Modeling a post-interaction binary¶
Contents:
- MESA@Konkoly – Massive Binaries
- Introduction
- Minilab 1: Stable Mass Transfer Evolution
- Minilab 2 (“Midilab”): The Efficiency of Mass Transfer
- Calibrating the Efficiency of Mass Transfer to an Observed System
- Varying the Mass Transfer Efficiency
- What Might Limit the Mass-Transfer?
- Ad hoc Model 1: Angular Momentum and Critical Rotation
- Implementation
- Checkpoint 0: Initialize a Global Variable to Store the Angular Momentum Accreted
- Checkpoint 1: Calculate AM accreted in
extras_binary_finish_step
- Checkpoint 2: Estimate the rotation rate
- Checkpoint 3: Calculate the critical rotation
- Checkpoint 4: Stop if the rotation rate is faster than critical rotation
- Run MESA binary with Ad Hoc Model 1 implemented!
- BONUS TASK: Ad hoc model 2: Thermal Timescale-limited accretion
- Solutions
- Maxilab: Towards the X-ray binary stage