Answer: Nothing significant.
Explanation: The energy flux emited by the sun will remain the same even if the sun's radius reduces drastically.
The energy from the sun reaching the Earth is given by the Stefan-Boltzmann equation.
Energy flux = Boltzmann's constant * T⁴
Energy flux = {{5.67*EXP(-8) watt per meter² per K⁴}*{5800K}⁴} = 63*EXP(6) Watt per meter²
Where EXP means 10^, and T= sun blackbody temperature 5800K.
It is good to know that the energy flux from the sun reaching the Earth does not depend on radius ( either it increases or decreases). The energy it supplies to earth remain the same.