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эритмалар. эритмалар назарияси. эритмаларнинг хоссалари
эритмалар. эритмалар назарияси. эритмаларнинг хоссалари

... When the process of isobaric pressure is constant: P = const For such a state of expression for the first law of thermodynamics Q =  U + р V is rewritten as follows: QP = U2 -U1 + р(V2 -V1) = U2 - U1 + рV2 -рV1 QP = (U2 + рV2) - (U1 - рV1) The thermal effect at constant pressure is called the enth ...
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Introduction to Heat Transfer

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saulvillalobos.files.wordpress.com

... for a reaction is equal in magnitude but opposite in sign to ΔH for the reverse reaction. The enthalpy change for a reaction depends on the state of the reactants and products. ...
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The work done on an object by an external force is given by the

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... The higher the charges on the ions that make up an ionic compound, the greater the (negative) lattice energy. Refer to table 8-3 on page 220 for some examples of lattice energies. Metallic Bonds and Properties of Metals Consider a sample of a metal. Although the atoms that make up that sample have v ...
entropy - Helios
entropy - Helios

... improbable event happening is absurdly low ...
ChE 215, Physical Chemistry
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... 1) Analysis of Organic Chemical solution using Gas Chromatograph. 2) To study the kinetics of hydrolysis of ethyl acetate solution to ethanol and acetic acid and to determine the reaction rate constant (K). 3) To study the adsorption isotherm using charcoal and acetic acid solution. 4) To determine ...
Bonding - Graham ISD
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... The only group that seldom forms compounds is the noble gases (group 18). This is true because compounds of these atoms are almost always less stable than the original atom. Atoms with a partially stable outer energy level can lose, gain, or share electrons to obtain a stable outer energy level. ...
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... What is meant by temperature? The Temperature of an object is a measure of the hotness or coldness of that object. What is the unit of temperature? The SI unit of temperature is the Kelvin (K) Give an example of a thermometric property. Resistance, length (of column of mercury), emf. The rise in tem ...
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Exam #: Printed Name: Signature: PHYSICS DEPARTMENT

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... ideal gas at constant volume so that its pressure drops from 2.2 atm to 1.4 atm. Then the gas expands at constant pressure, from a volume of 6.8 L to 9.3 L, where the temperature reaches its original value. Calculate (a) the total work done by the gas in the process, (b) the change in internal energ ...
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GCSE Physics criteria sheet

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... We understand that Eeff is conserved because it is the energy in an analogue problem in which the test particle moves in the gravitational field of a point particle of mass M (ri ), located at the origin, with potential energy function Veff (r). In this analogue problem the force on the test particle i ...
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... • The number of atoms of each type of element on the reactant side (left of the arrow) must be equal those on the product side (right side of the arrow). 2 H2 + O2 2 H2O • There are 4 hydrogen atoms on the left (2 H2) and 4 hydrogen atoms on the right (2 H2O) • There are 2 atoms of oxygen (O2) on th ...
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Chapter 12

... An isolated system does not interact with its surroundings No energy transfer takes place and no work is done Therefore, the internal energy of the isolated system remains constant ...
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Heat transfer physics



Heat transfer physics describes the kinetics of energy storage, transport, and transformation by principal energy carriers: phonons (lattice vibration waves), electrons, fluid particles, and photons. Heat is energy stored in temperature-dependent motion of particles including electrons, atomic nuclei, individual atoms, and molecules. Heat is transferred to and from matter by the principal energy carriers. The state of energy stored within matter, or transported by the carriers, is described by a combination of classical and quantum statistical mechanics. The energy is also transformed (converted) among various carriers.The heat transfer processes (or kinetics) are governed by the rates at which various related physical phenomena occur, such as (for example) the rate of particle collisions in classical mechanics. These various states and kinetics determine the heat transfer, i.e., the net rate of energy storage or transport. Governing these process from the atomic level (atom or molecule length scale) to macroscale are the laws of thermodynamics, including conservation of energy.
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