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PHYSICAL SCIENCE
NUCLEAR REACTION AND ALPHA DECAY
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Nuclear reaction
Process in which a nucleus either combines with another nucleus (nuclear fusion) or splits into a smaller nuclei (nuclear fission)
Nuclear reaction
1. A nucleus combines with another nucleus (nuclear fusion) or splits into a smaller nuclei (nuclear fission)
2.
Emission
of
energetic
particles of an atom
Radioactivity
Emission of energetic particles of an atom
Alpha
Decay
Loss of an alpha particle
Beta
decay
loss of a beta particle
Gamma radiation
emission of gamma ray
Positron Emission
conversion of a proton in a nucleus into neutron along with the release of a positron
Electron Capture
drawing of an electron into an atom molecules
The universe may have begun as an infinitely hot and dense initial
singularity
, a point with all of
space
,
time
,
matter
and
energy
Inflation
The universe cooled down as it expanded
Protons and neutrons came together to form different types of nuclei by nucleosynthesis or nuclear fusion
Recombination
Electrons started to bind to ionized protons and nuclei forming neutral atoms
Formation of stars and galaxies
Gravity
caused these atoms to collapse onto one another to form stars and galaxies
Eventually,
stars
and
galaxies
formed other matter
Redshift
Stars and galaxies shine with light shifted toward the red end of the spectrum
Light waves of cosmic bodies
Stretched into
low frequency red waves
as they move away from an observer on Earth
Stars
Made up of hydrogen, become hotter and denser
Stellar formation and evolution
Light elements
combined to form
Carbon
,
Neon
,
Oxygen
,
Silicon
,
Iron
Young stars
Small
Yellow
Nuclear reactions
Occurred successively until it became a
giant
red
star
Stars such as the sun have a temperature of less than
15 million
Kelvin
CNO Cycle
A process through which Carbon (12C) serves as a catalyst to form other elements
CNO Cycle
1.
Proton
capture
2.
Beta
decay
SUPERNOVA
SUPERNOVA
1. Explosion that releases a tremendous amount of energy
2. Synthesizes elements heavier than
iron
r
process
Rapid capture of neutrons by the atom
s
process
Slow neutron capture in red giants