'Nuclear force' diaporamas de présentation

Warmup

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Chapter 29

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Chapter 29

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In the God Particle We Trust (?): Understanding the Collisions, Emissions & Omissions

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CHAPTER 30

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Evidence of God

- newmanlib.ibri.org -. Evidence of God. In Cosmos & Conscience Robert C. Newman. Abstracts of Powerpoint Talks. The Biblical Claim. - newmanlib.ibri.org -.

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PSC 4010

PSC 4010. Nuclear Technology: A matter of Energy. PSC 4010: Chapter 2. Goals: _ SWBAT put the different atomic theories in a historical and technical context _SWBAT compare the current simplified atomic model with all precedent models and theories. PSC 4010: Chapter 2.

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Lesson 5

Lesson 5. Fundamental Aspects of Nuclear Structure. Fundamental Forces of Nature. Exchange Particles and Force Carriers. Forces occur through the notion of the virtual exchange of bosons that are force carriers.

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Where did Elements come from?

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The Atom

The Atom. Prepared by: Timothy John D. Matoy. The Atom. The atom is the smallest particle that has all the properties of an element. Greek atom. Dalton Atom. 1808. ThomPson Model. 1890. Rutherford Model. 1911. Bohr Model. 1913. Atomic Structure. Atomic Notation. z X A

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Utilitarianism

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Exploring the Early Universe

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CHAPTER 12 The Atomic Nucleus

CHAPTER 12 The Atomic Nucleus. 12.1 Discovery of the Neutron 12.2 Nuclear Properties 12.3 The Deuteron 12.4 Nuclear Forces 12.5 Nuclear Stability 12.6 Radioactive Decay 12.7 Alpha, Beta, and Gamma Decay 12.8 Radioactive Nuclides.

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Solar system: 9 light hours diameter

Solar system: 9 light hours diameter. Spiral galaxy: 80,000 light years diameter. Coma cluster of galaxies: 2.5 million light years across. Survey of distant galaxies: 5 to 9 billion light-years away.

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Modern Physics

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The Sun, Earth, and Moon

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Fusion

Fusion. Light Nuclei. Light nuclei have relatively high rest masses. H-1: 1.008665 u H-2: 2.014102 u He-3: 3.016029 u He-4: 4.002603 u C-12: 12.000000 u Energy is available compared to heavy mass nuclei. Si-28: 27.976926 Fe-56: 55.934942.

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Forces of Nature

Newton's Laws of Motion Inverse square law of forces Fundamental forces (4). Forces of Nature. (3) Weak nuclear force Example: ?-decay or top bottom quark (4) Strong nuclear force Example: force that binds protons & neutrons in atomic nuclei.

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Standard Model of Particles

Standard Model of Particles. TIME. SPACE. Strong Interaction. E&M Interaction. Hadronic Interaction (residual nuclear force). Weak Interaction. Symmetries. Continuous Symmetries space-time translation rotational invariance Lorentz boosts gauge invariance

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