Transfer of energy by electromagnetic waves
e.g. Sun keeps earth warm
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thermodynamics
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a branch of physics concerned with heat and temperature and their relation to energy and work. It defines macroscopic variables, such as internal energy, entropy, and pressure, that partly describe a body of matter or radiation.
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plasma
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an ionized gas consisting of positive ions and free electrons in proportions resulting in more or less no overall electric charge, typically at low pressures (as in the upper atmosphere and in fluorescent lamps) or at very high temperatures (as in stars and nuclear fusion reactors).
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First law of thermodynamics
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The change in the total internal energy of a system is equal to the amount of energy transferred in the form of heat to the system, minus the amount of energy transferred from the system in the form of work
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heat engine
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a device for producing motive power from heat, such as a gasoline engine or steam engine.
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Four special types of thermodynamic systems in which a given variable is held constant
During a phase change, heat energy causes changes in PE and energy distribution, but not KE. No change in temp
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Heat of transformation equation
Front
q= amount of heat gained or lost from substance
m= mass
L= heat of transformation
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conduction
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the process by which heat or electricity is directly transmitted through a substance when there is a difference of temperature or of electrical potential between adjoining regions, without movement of the material.
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absolute zero
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the lowest temperature that is theoretically possible, at which the motion of particles that constitutes heat would be minimal.
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Thermodynamics
Front
Flow of energy in the universe, as the flow relates to work, heat, entropy, and the different forms of energy
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Closed systems
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System capable of exchanging energy, but not matter, with the surrounding
e.g. gas in vessels with movable pistons
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Zeroth law of thermodynamics
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Objects are in thermal equilibrium when they are at the same temperature, transitive property in thermal systems (a=b, b=c, a=c)
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Heat gained or lost by an object
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q= heat gained or lost by an object
m= mass
c= specific heat of substance
delta T= change in temp
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Convection
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Transfer of heat by the physical motion of a fluid over a material
e.g. Fans circulate hot air inside oven
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Entropy
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Measure of how much energy has spread out or how spread out energy has become
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Carnot cycle
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an ideal reversible closed thermodynamic cycle; back to it's original state
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deposition
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when an object goes from a gas straight to solid, without going through a liquid phase
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heat
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a form of energy associated with the movement of atoms and molecules in any material.
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Carnot engine
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most efficient heat engine, uses two isothermal and two adiabatic processes
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Specific heat (c) of a substance
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The amount of heat energy required to raise one gram of a substance by one degree Celsius or one unit Kelvin
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radiation
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the emission of energy as electromagnetic waves or as moving subatomic particles, especially high-energy particles that cause ionization.
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Adiabatic process
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No heat is exchanged
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Isothermal process
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T is constant, change in internal energy= 0
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Isovolumetric (isochoric) process
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V is constant, work done on or by system = 0
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Thermal expansion
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delta L= change in length
alpha= coefficient of linear expansion
L= original length
delta T= change in temperature
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Heat
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The transfer of thermal energy from a hotter object(higher temp/energy) to a colder object (lower temp/energy)
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Second law of thermodynamics
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In a closed system, energy will spontaneously and irreversibly go from being localized to being spread out
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internal energy
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the energy in a system arising from the relative positions and interactions of its parts.
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Thermal equilibrium
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No heat flows between two objects in thermal contact
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Kelvin to Celsius equation
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Fahrenheit to Celsius equation
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convection
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the movement caused within a fluid by the tendency of hotter and therefore less dense material to rise, and colder, denser material to sink under the influence of gravity, which consequently results in the transfer of heat.
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First law of thermodynamics equation
Front
delta U= internal energy
Q= heat
W= work
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Conduction
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Direct transfer of energy from molecule to molecule through molecular collisions
e.g. metal pan to chicken, gases are poor conductors
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Isolated systems
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System not capable of exchanging energy or matter with their surrounding; total change in internal energy is zero
e.g. bomb calorimeter
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State functions
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Thermodynamic properties that are a function of only the current equilibrium state of a system
e.g. pressure, density, temperature, volume, enthalpy, internal energy, Gibbs free energy, entropy
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isothermal
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a change of a system, in which the temperature remains constant
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Entropy and heat
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delta S= change in entorpy
Q rev= heat gained or lost in reversible process
T= temperature
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Three means by which heat can transfer energy
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Conduction, Convection, Radiation
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Open systems
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Systems can exchange both matter and energy with the environment
e.g. Boiling pot of water
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entropy
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lack of order or predictability; gradual decline into disorder. // a thermodynamic quantity representing the unavailability of a system's thermal energy for conversion into mechanical work, often interpreted as the degree of disorder or randomness in the system.
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Temperature
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A physical property of matter that relates the average kinetic energy of the particles in a substance
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sublimation
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a transition of a substance directly from the solid to the gas phase without passing through the intermediate liquid phase
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Isobaric process
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P is constant
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adiabatic
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relating to or denoting a process or condition in which heat does not enter or leave the system concerned.
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mole
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the SI unit of amount of substance, equal to the quantity containing as many elementary units as there are atoms in 0.012 kg of carbon-12.
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Entropy of universe
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This total entropy of the universe is always increasing
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isochoric
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a thermodynamic process during which the volume of the closed system undergoing such a process remains constant.
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Section 2
(7 cards)
calorie
Front
the energy needed to raise the temperature of 1 kilogram of water through 1 °C, equal to one thousand small calories and often used to measure the energy value of foods.