CM

chapter 10-16 core concepts

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## Chapter 10: The Decline of the Aristotelian Worldview

Historical Context:

* Aristotelian worldview dominated European thought for ~1500 years.

* Earth-centered universe; celestial spheres made of perfect “aether”; immutable heavens.

* Science intertwined with theology: final causes (purpose) and natural order dictated motion.

Key Concepts:

* Geocentric Model: Earth is the universe’s center; planets and stars move in perfect circles.

* Natural Motion: Objects move toward their “natural place” (stone falls, fire rises).

* Celestial Perfection: Heavenly bodies move uniformly; change only occurs on Earth.

Challenges:

* Copernicus (1473–1543): Heliocentric model; mathematical simplicity but controversial.

* Galileo (1564–1642): Telescopic discoveries—moons of Jupiter, phases of Venus, sunspots—disproved immutability.

* Kepler (1571–1630): Planetary orbits are elliptical, not circular.

Philosophical Implications:

* Empirical observation challenges authority and tradition.

* Mathematics becomes essential for describing nature.

Emergence of *scientific methodology**: hypothesis, observation, experiment.

Example: Galileo observing moons of Jupiter → empirical proof that not everything orbits Earth.

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## Chapter 11: The Newtonian Worldview

Historical Context:

* 17th-century Europe: Scientific Revolution; shift from qualitative to quantitative understanding.

* Newton (1642–1727) synthesizes laws of motion and universal gravitation.

Key Concepts:

* Newton’s Laws of Motion:

1. Inertia: objects at rest stay at rest unless acted upon.

2. F=ma: force = mass × acceleration.

3. Action-reaction: every action has an equal opposite reaction.

* Universal Gravitation: All objects attract; explains planetary motion.

Philosophical Impacts:

* Deterministic universe: predictable, mechanical, “clockwork universe.”

* Mechanistic explanation replaces Aristotelian teleology.

* Reinforced empiricism: observation and mathematics as primary tools.

Key Terms: absolute space and time, mechanistic universe.

Example: Predicting the path of planets using Newton’s equations.

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## Chapter 12: Scientific Laws and Their Status

Key Concepts:

* Scientific Law: Empirical generalization describing natural phenomena.

* Types:

* Descriptive: summarize patterns (e.g., Kepler’s laws).

* Explanatory: describe cause-effect relationships (Newton’s laws).

Philosophical Debates:

* Realism: Laws describe reality as it is.

* Instrumentalism: Laws are tools for prediction, not necessarily “true.”

* Nomological vs. Phenomenal Laws: Do laws exist or just describe observations?

Examples:

* Newton’s law of gravitation (realist interpretation: force exists).

* Thermodynamics (predictive; instrumentalist view may suffice).

Implications:

* Determines the role of science in explaining vs. predicting.

* Raises questions about universality vs. context-dependence of laws.

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## Chapter 13: The Challenge of Evolutionary Theory

Historical Context:

* Pre-Darwin: species considered fixed; teleological explanations dominate.

* Darwin (1809–1882): species evolve over time via natural selection.

Key Concepts:

* Natural Selection: Variation, inheritance, differential survival.

* Adaptation: Traits that improve survival become more common.

* Speciation: Gradual divergence leads to new species.

Controversy:

* Challenges religious and Aristotelian views of fixed life forms.

* Social and ethical implications: human nature, morality, purpose.

Philosophical Questions:

* Determinism vs. chance in evolutionary processes.

* Teleology vs. naturalistic explanation: Is there purpose in nature?

Example: Darwin’s finches in the Galápagos Islands—beak shapes adapted to environment.

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## Chapter 14: The Rise of Quantum Theory

Historical Context:

* Early 20th century: classical physics cannot explain atomic phenomena.

Key Concepts:

* Wave-Particle Duality: Light and matter exhibit both wave and particle properties.

* Heisenberg Uncertainty Principle: Limits of measuring position and momentum simultaneously.

* Probabilistic Nature: Quantum mechanics predicts probabilities, not certainties.

Philosophical Interpretations:

* Copenhagen Interpretation: Reality depends on measurement.

* Hidden Variables: Suggests determinism may still exist.

* Many-Worlds: All possible outcomes occur in branching universes.

Impact:

* Challenges classical determinism.

* Redefines notions of reality, causality, and observation.

Key Figures: Planck, Einstein (critic), Bohr, Heisenberg, Schrödinger.

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## Chapter 15: The Theory of Relativity

Historical Context:

* Early 20th century: Newtonian mechanics fails at high speeds or strong gravity.

* Einstein (1879–1955) develops relativity theory.

Key Concepts:

* Special Relativity:

* Laws of physics same in all inertial frames.

* Constant speed of light.

* Time dilation, length contraction.

* Mass-energy equivalence (E=mc²).

* General Relativity:

* Gravity is curvature of spacetime.

* Massive objects distort spacetime.

Philosophical Implications:

* Absolute space and time replaced by relative spacetime.

* Challenges intuitive notions of reality.

Impact:

* Practical: GPS adjustments for time dilation.

* Theoretical: Black holes, cosmology, early universe physics.

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## Chapter 16: The Contemporary Scientific Worldview

Core Concepts:

* Integration of Quantum Mechanics and Relativity: Ongoing challenge.

* Complexity Theory: Emergent behavior from interacting systems.

* Chaos Theory: Sensitive dependence on initial conditions; deterministic yet unpredictable.

Philosophical Reflections:

* Limits of scientific explanation; science evolves continuously.

* Science as probabilistic, approximate, and interconnected.

* Recognition of uncertainty and model-dependence.

Examples:

* Climate modeling (complex systems).

* Particle physics (quantum uncertainty + relativity).