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7.2- Nuclear reactions (PPT)
7.2- Nuclear reactions (PPT)

... Nuclear fusion ▪ For a more massive star, there is enough gravity to fuse the elements all the way up to iron. ▪ But there can be no more fusion when the star is completely iron. Why? ▪ Since the radiation pressure now ceases, gravity is no longer balanced and the star collapses into a neutron star ...
Lecture - 1
Lecture - 1

sch3u unit 1 test: matter
sch3u unit 1 test: matter

... 9. When fluorine forms an ionic bond it tends to a. lose electrons b. gain electrons c. share electrons d. lose protons 10. Copper (II) hydroxide is composed of a. 2 elements, 2 atoms b. 2 elements, 3 atoms c. 3 elements, 4 atoms d. 3 elements, 5 atoms ...
NUCLEAR CHEMISTRY
NUCLEAR CHEMISTRY

2DCAtStrUT2010
2DCAtStrUT2010

(neutron/proton ratio is 1).
(neutron/proton ratio is 1).

NUCLEAR CHEMISTRY: INTRO
NUCLEAR CHEMISTRY: INTRO

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Chemical Change

... The chemical properties of elements are related to the energy changes that take place when atoms lose, gain or share electrons to obtain a filled valence shell. ...
Nuclear Chemistry Radioactivity
Nuclear Chemistry Radioactivity

particle - Uplift North Hills
particle - Uplift North Hills

... Neutrinos are elementary particles that travel close to the speed of light, lack an electric charge, are able to pass through ordinary matter almost undisturbed and are thus extremely difficult to detect It took 26 years before the neutrino was actually detected. As of 1999, it is believed neutrinos ...
Click here for printer-friendly sample test questions
Click here for printer-friendly sample test questions

File
File

... • nuclei fuse together • for very light elements, stability increases with increasing mass ...
Atomic Structure Notes
Atomic Structure Notes

... Dalton’s Atomic Theory (1808) 1. Elements are composed of extremely small particles called atoms. 2. All atoms of a given element are identical, having the same size, mass and chemical properties. 3. The atoms of one element are different from the atoms of all other elements. 4. Atoms of one elemen ...
Nuclear and Radiation Section - University of Toronto Physics
Nuclear and Radiation Section - University of Toronto Physics

... necessary to postulate another force of nature - the so-called strong force – that comes into play only at a distance of less than 10-15 m or so. This very short-range strong force does not distinguish between neutrons and protons, being attractive between any two nucleons (p-p, p-n, n-n); it is the ...
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Practice_Final_B

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... c. Which quantum number (n, l, ml or ms) describes the quantization of the direction of an electron's orbital angular momentum? d. When the electrons in a substance bind into Cooper pairs, what does the substance become? e. Classical physics and the equipartition theorem predict the specific heat of ...
Radioactivity2015
Radioactivity2015

... • This particle, which consists of two protons and two neutrons, has a net positive charge. • Although emitted with high energy, alpha particles lose energy quickly as they pass through matter of air and therefore, do not travel long distances. • They can even be stopped by a piece of paper or the o ...
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Resource Lesson Nuclear Reaction When we speak of atoms, we

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Nuclear Astrophysics (1)

... this leads to the following abundance relations ...
File - Mr. Walsh`s AP Chemistry
File - Mr. Walsh`s AP Chemistry

... named by describing the molecular formula, using prefixes for the numbers. o You will need to memorize the number prefixes for the numbers 1–10. o E.g., P2O5 is diphosphorus pentoxide. **Note that the prefix “mono—“ is never used with the first element. SO3 is simply sulfur trioxide. However, “mono— ...
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Additional Problems - AppServ Open Project 2.4.9

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Standard 2 Key

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... made of matter has mass  Most of the mass of an atom is found in the nucleus • About 99.9% of the mass of an atom is in the nucleus Nuclear Particles  The two particles in the nucleus, protons and neutrons, make up 99.9 % of the mass of the atom ...
South Pasadena · AP Chemistry
South Pasadena · AP Chemistry

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Nuclear binding energy

Nuclear binding energy is the energy that would be required to disassemble the nucleus of an atom into its component parts. These component parts are neutrons and protons, which are collectively called nucleons. The binding energy of nuclei is due to the attractive forces that hold these nucleons together and this is usually a positive number, since most nuclei would require the expenditure of energy to separate them into individual protons and neutrons. The mass of an atomic nucleus is usually less than the sum of the individual masses of the constituent protons and neutrons (according to Einstein's equation E=mc2) and this 'missing mass' is known as the mass defect, and represents the energy that was released when the nucleus was formed.The term nuclear binding energy may also refer to the energy balance in processes in which the nucleus splits into fragments composed of more than one nucleon. If new binding energy is available when light nuclei fuse, or when heavy nuclei split, either process can result in release of this binding energy. This energy may be made available as nuclear energy and can be used to produce electricity as in (nuclear power) or in a nuclear weapon. When a large nucleus splits into pieces, excess energy is emitted as photons (gamma rays) and as the kinetic energy of a number of different ejected particles (nuclear fission products).The nuclear binding energies and forces are on the order of a million times greater than the electron binding energies of light atoms like hydrogen.The mass defect of a nucleus represents the mass of the energy of binding of the nucleus, and is the difference between the mass of a nucleus and the sum of the masses of the nucleons of which it is composed.
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