BioPhysics Lecture - Heat and Thermal Properties

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This set covers temperature measurement, thermal expansion types and formulas, heat transfer mechanisms (conduction, convection, radiation), and specific heat calculations based on the lecture notes.

Last updated 7:53 AM on 6/1/26
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17 Terms

1
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Heat stops transferring between bodies when __________ is reached.

thermal equilibrium

2
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The formula for the Platinum thermometer relates resistance and temperature as __________.

R=R0(1+αΔT)R = R_0 (1 + \alpha \Delta T)

3
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The General Thermometer Equation used to calculate temperature based on a property XX is __________.

T=XX0X100X0×100T = \frac{X - X_0}{X_{100} - X_0} \times 100

4
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The three types of thermal expansion are longitudinal, area, and __________.

Volume

5
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The relationship between the linear expansion coefficient (α\alpha) and the volume expansion coefficient (γ\gamma) is __________.

γ=3α\gamma = 3\alpha

6
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The unit for the thermal expansion coefficient is __________.

C1^{\circ}C^{-1}

7
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For a material to expand uniformly in all dimensions, it must be a __________ material.

Homogenous

8
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The amount of energy needed to raise the temperature of 1g1\,g of water by 1C1^{\circ}C is defined as a __________.

Calorie

9
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The heat required for a phase change without a change in temperature is called __________.

Latent heat

10
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In a thermostat comprising steel and brass, the metal __________ must have a higher thermal expansion coefficient.

Brass

11
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The method of measuring the specific heat of a solid body described in the notes is the __________.

mixing method

12
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The three methods of heat transfer are conduction, convection, and __________.

Radiation

13
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Heat transfer in solids occurs primarily through __________.

Conduction

14
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The rate of heat transfer by conduction is given by the formula __________.

H=KAΔTLH = -K \cdot A \cdot \frac{\Delta T}{L}

15
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An ideal body that absorbs all incoming light and redistributes it is known as a __________.

Black body

16
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For an ideal Black body, the emissivity (ϵ\epsilon) is equal to __________.

11

17
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The Stefan-Boltzmann constant (σ\sigma) used in radiation calculations is __________.

5.67×108W/m2K45.67 \times 10^{-8}\,W/m^2\cdot K^4