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In this Physics video in Hindi we explained Stefan-Boltzmann law for blackbody radiation for class 11. Every body emits energy, which depends upon its surface area, temperature and emissivity. This law states that the energy emitted by a body per second is the product of the emissivity of that body, the Stefan-Boltzmann constant, the surface area of the body and the fourth power of the absolute temperature of that body.
🔴 Click here to watch the whole playlist on 'Thermal Properties of Matter' for Class 11 :
• Thermal Properties of ...
Previous videos -
🔴 Thermal Properties of Matter - Introduction || in HINDI for Class 11
• Thermal Properties of ...
🔴 Temperature and Heat
• 🔴 Temperature and Heat...
🔴 Measurement of Temperature || for Class 11 in HINDI
• 🔴 Measurement of Tempe...
🔴 Ideal Gas Equation and Absolute Temperature || for Class 11 in HINDI
• 🔴 Ideal Gas Equation a...
🔴 Kelvin Scale of Temperature
• 🔴 Kelvin Scale of Temp...
🔴 THERMAL EXPANSION
• Thermal Expansion || f...
🔴 Relation among Coefficients of Thermal Expansion
• Relation among Coeffic...
🔴 THERMAL STRESS || in HINDI
• THERMAL STRESS || in H...
🔴 Anomalous Thermal Expansion of Water
• 🔴 Anomalous Thermal Ex...
🔴 Coefficient of Volume Expansion of Gas
• 🔴 Coefficient of Volum...
🔴 Heat Transfer
• 🔴 Heat Transfer || for...
🔴 Conduction and Thermal Conductivity
• 🔴 Conduction and Therm...
🔴 Convection
• 🔴 Convection || for Cl...
🔴 Radiation || for Class 11 in HINDI
• 🔴 Radiation || for Cla...
🔴 Wien's Displacement Law for Blackbody Radiation
• 🔴 Wien's Displacement ...