Nuclear Force and Particles

Slides:



Advertisements
Similar presentations
Chapter 22 – Nuclear Chemistry
Advertisements

Unit 2 Notes – Radioactivity
Transmutations involve more than just the conversion of one element into another—they also involve the conversion of mass into energy. Nuclear energy released.
20th Century Discoveries
Einstein’s Energy Mass Equivalence Powers the Sun!
Lecture 14 Fission and Fusion. Elementary Particles. Nuclear Fission Nuclear Fusion Fundamental Interaction (Forces) Elementary Particles.
Fundamental Forces of the Universe
Nuclear Energy Nuclear Reactions Nuclear Fission / Nuclear Fusion Harnessing the Power of the Nucleus.
Section 2Nuclear Changes Nuclear Forces 〉 What holds the nuclei of atoms together? 〉 The stability of a nucleus depends on the nuclear forces that hold.
The equation E = mc 2 is probably the most recognized symbol of physics. This equation tells us that matter and energy are really two forms of the same.
Chapter 9 Notes.  While chemical changes involve changes in the electrons (ex : bonding), nuclear reactions involve changes to the nucleus and involve.
Nuclear Fission and Fusion
Nuclear Physics E = mc 2. Outline Theory of Special Relativity Postulates E = mc 2 The Atom What makes up the atom? What holds the atom together? Quantum.
Fusion Energy. Source of Energy Before 1940 the Sun’s energy was a mystery.  Chemical reactions:  Gravitational energy:  Nuclear forces: The Sun is.
Radiation, nuclear fusion and nuclear fission
Nuclear Physics. Nuclear Physics is the study of the atom. This is a larger part of modern physics study, however we will only look at basic energy exchanges.
Nuclear Fission and Fusion
NUCLEAR FUSION NUCLEAR FISSION. chools/gcsebitesize/scie nce/add_aqa/atoms_rad iation/nuclearact.shtmlhttp:// chools/gcsebitesize/scie.
C HAPTER 10: R ADIOACTIVITY The process of Transmutation plus 10.4 Fission and Fusion.
Unit 8 Section 2: Nuclear Reactions
Section 10–4: Fission and Fusion
Structure and Stability of Nuclei, Fission, Fusion, and Radiation
Nuclear Forces How do you keep a bunch of Protons together?
"More than any other time in history, mankind faces a crossroads. One path leads to despair and utter hopelessness. The other, to total extinction. Let.
Nuclear Chemistry.
Subatomic Physics Chapter Properties of the Nucleus The nucleus is the small, dense core of an atom. Atoms that have the same atomic number but.
Atomic Stability. Isotopes Isotopes are atoms of an element that have different numbers of neutrons in their nucleus. Cu Copper – 63 OR Copper.
Topic – Physics 2a Mass defect and binding energy Prior learning Atomic structure Electrical forces Key words –Atomic nucleus,mass difference, mass of.
Section 10–4: Fission and Fusion Physical Science Coach Kelsoe Pages 308–315.
Modern Physics. Answer Me!!! How much energy does a photon have if the light beam has a wavelength of 720 nm?
Nuclear Power. Locations of Nuclear Power plants in the US.
Unit 12 – Nuclear Chemistry. Part II Key Terms Alpha decay – spontaneous decay of a nucleus that emits a helium nucleus and energy Beta decay – spontaneous.
Fundamental Forces of the Universe. There are four fundamental forces, or interactions in nature.  Strong nuclear  Electromagnetic  Weak nuclear 
Aim: How can we explain the four fundamental forces and the standard model? Do Now: List all the subatomic particles that you can think of.
3-4 Changes in the Nucleus
The Nucleus Nucleons- the particles inside the nucleus: protons & neutrons Total charge of the nucleus: the # of protons (z) times the elementary charge.
Nuclear Radiation 9.2. The Nucleus Protons and neutrons Charge of electrons and protons – x C = e –Proton +e –Electron -e.
Modern Physics. Reinventing Gravity  Einstein’s Theory of Special Relativity  Theorizes the space time fabric.  Describes why matter interacts.  The.
Nuclear Reactions and Radioactivity Part II
Nuclear Physics.
Nuclear Fission and Fusion Unit 8 – Part B. Nuclear Balance Delicate balance between attractive strong nuclear forces and repulsive electric forces. In.
7.2 Nuclear Fission and Fusion. Nuclear Fission Why are some elements radioactive? There is an optimal ratio of neutrons to protons 1 : 1 for smaller.
Mass-Energy Equivalence All matter is a form of stored energy.
Nuclear Reactions: FISSION & FUSION ã Nuclear reactions deal with interactions between the nuclei of atoms ã Both fission and fusion processes deal with.
Nuclear Reactions. Nuclear Symbols Element symbol Mass number (p + + n o ) Atomic number (number of p + )
Chapter 14 Section 14.1.
N UCLEAR C HEMISTRY Chapter 28. N UCLEAR FORCE - WHAT HOLDS THE ATOM TOGETHER Two opposing forces in the nucleus: Electrostatic- proton vs proton repulsion.
Unit 3: Part 2 of the Atom Nuclear Chemistry I. The Nucleus (p. 701 – 704 in Class Modern Chemistry Text) I. The Nucleus (p. 701 – 704 in Class Modern.
Fusion The reason we have life on Earth. Expectation #8: Definition A nuclear reaction in which smaller atomic nuclei collide at high speed to make a.
Unit 13: The nucleus of an atom We know that atoms are composed of electrons, protons and neutrons. Protons and neutrons together (i.e. the nucleus) are.
Chapter 10 Nuclear Decay. Objectives 〉 What happens when an element undergoes radioactive decay? 〉 How does radiation affect the nucleus of an unstable.
II. The Nucleus of the Atom. What makes up the nucleus of an atom? A. Compostion (Nucleons) 1. Protons a. Mass universal mass units b. Indicated.
Fission and Fusion are both nuclear reactions that involve the particles in the nucleus of an atom.
Fission and Fusion Physics 12 Adv. Nuclear Particles As we discussed, the nuclear particles are composed of quarks; the individual particles are the result.
Nuclear Fission and Fusion Chapter 10.2 Notes. Nuclear Forces Protons and neutrons are tightly packed inside the nucleus Remember that unstable nuclei.
Nuclear Fission and Fusion Notes. November 3, 2008 What part of the atom is affected by Nuclear Chemistry? Do you think the benefits of nuclear energy.
Nuclear Energy.
The Standard Model of Particle Physics
Chapter 9.2 Nuclear Radiation.
The Standard Model An Introduction to Particle Physics
A. Nuclear Forces Do nuclei contain attractive or repulsive forces?
A. Nuclear Forces Do nuclei contain attractive or repulsive forces?
E = mc2 If you can’t explain it simply, you haven’t learned it well enough. Einstein.
Fundamental Forces of the Universe
Where did the energy for this come from?
Fundamental Forces of the Universe
Unit 3: Part 2 of the Atom Nuclear Chemistry
Nuclear Energy.
Fundamental Forces of the Universe
Nuclear Chemistry Chapter 28.
Presentation transcript:

Nuclear Force and Particles Principles of Physics

Models of the Atom Understanding of wave-particle duality led to better understanding of the atom It was determined that the protons and neutrons occur together in the center with electrons orbiting it at various locations But, how does the nucleus stay together when it is made up of like and neutral charges???

Nuclear Forces Strong Force: – attractive force between particles in nucleus Keeps nucleus stable 100 x stronger than the electrostatic force only effective at small distances (short range) breaking “bonds” – releases a lot of energy

Nuclear Force Weak force: responsible for the radioactive decay Weaker than strong and electromagnetic forces For large atoms the strong force is not always strong enough to hold the nucleus together The weak force breaks the atom into smaller more stable atoms while releasing energy The weak force is responsible for such things as the sun being able to produce energy and carbon dating

Einstein’s Mass-Energy Equation Mass is another form of energy. To find the mass equivalent of energy we use Einstein’s famous equation:   E=mc2    E = energy (J) m = mass (kg) c = speed of light in a vacuum = 300,000,000 m/s

Mass-Energy Conversions Example: Energy from the sun is produced through radioactive decay. The sun’s mass is being converted into energy. As the Sun’s energy comes to Earth , it’s mass will continue to decrease. Example: During chemical reactions when atoms combine the sum of the mass of the individual atoms before the reaction is not equal to the mass of the combined atoms after the reaction. The excess mass was converted to energy.

Fission Fission: splitting of large atoms resulting in the release of energy The energy released is related to the mass lost through E= mc2 Fission can occur as a chain reaction Atomic bomb Nuclear reactors

Fusion Fusion: Combining of small atoms to make larger ones and a release of energy The energy released is related to the mass lost through E= mc2 Fusion requires a huge amount of energy to activate The sun and stars produce energy through fusion No successful fusion reactors exist on Earth, because of the conditions necessary to activate the reaction

Elementary Particles Although it was believed for a very long time that protons, neutrons, and electrons were the smallest particles, they were wrong… Types of particles 1. Baryons (include protons and neutrons) Made up of three smaller particles called quarks 2. Mesons Made up of two quarks 3. Leptons (include electrons and neutrinos) 4. Bosons

Antimatter Antimatter: Matter that has all the same properties as the regular matter except the electric charge is reversed Example: positron (anti-electron), has the same mass as an electron, but is positively charged Antimatter does not occur in the natural universe as far as we know. It can be created in labs in very small quantities.

Matter – Antimatter Interactions When a particle and an antiparticle meet, both are turned into pure energy   Matter – antimatter reactions are the most energetic reactions in the known universe Example: If 500 kg of water were added to 500 kg of anti-water, the energy released would be able to power the entire US for a year!!