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The Second Law of Thermodynamics, a fundamental principle in physical science, asserts that the entropy of an isolated system will increase over time. This law is rooted in statistical mechanics and applies to the behavior of particles in a system, predicting a natural progression towards equilibrium. It also plays a crucial role in understanding the Big Bang, the development of the universe, the thermodynamics of living organisms, and the concept of the arrow of time. Gravitational systems and non-equilibrium states further illustrate the law's implications.
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Entropy is a measure of disorder or randomness in a system, calculated using Boltzmann's constant and the number of microstates
Most Probable State
The Second Law states that the most probable state for a system is one of maximum entropy, reflecting the highest number of microstates consistent with the macroscopic constraints
Equilibrium
The Second Law applies to future predictions and states that the entropy of an isolated system not in equilibrium will tend to increase over time, approaching a maximum value at equilibrium
The Second Law is silent on the past, except when additional information confirms a lower entropy state previously
Boltzmann's constant (k_B) is used in the formula for calculating entropy
Entropy is calculated using the number of microstates (Ω) corresponding to the macrostate of the system
Entropy changes when energy is transferred or when the system's volume or other external conditions change, leading to a redistribution of microstates
Reversible processes occur infinitely slowly, allowing the system to remain in equilibrium at all times
For reversible processes, the change in entropy (dS) is directly proportional to the heat added to the system (δQ) and inversely proportional to the temperature (T)
The relationship between entropy change, heat, and temperature is a manifestation of the fundamental link in thermodynamic systems
The Big Bang theory suggests that the universe began in a state of extremely low entropy, setting the initial conditions for the Second Law of Thermodynamics
The simplicity and uniformity of the early universe have given way to increasing complexity and higher entropy states
Theories such as cosmological inflation aim to explain the initial conditions of the universe and its ongoing evolution