How does energy transfer in the radiative zone compare to that in the convective zone?
Current stellar models assume all heat transfer is primarily by radiation, with negligible convection (in cooler stars).
Here is the link to the most lucid explanation and comparison I could find: https://tutor.hix.ai
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Energy is transferred by electromagnetic radiation in the radiative zone and physically by the movement of hot plasma in the convective zone.
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When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
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