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1 Abundance anomalies in RGB stars
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2 From the pioneering work on stellar rotation to the present
treatment of the transport of angular momentum and chemicals
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3 Physical inputs for the evolution of rotating stars
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4 Numerical simulations
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5 Testing the physics of rotation
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6 Signatures of mixing
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7 Comparison with previous works
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8 Conclusion
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Appendix A: Detailed expressions for the components
and 
in Eq. (2)
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References
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