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Nuclear physics
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From Wikipedia, the free encyclopedia
Nuclear physics
Nucleus
Nucleons
p
n
Nuclear matter
Nuclear force
Nuclear structure
Nuclear reaction
Models of the nucleus
Liquid drop
Nuclear shell model
Interacting boson model
Ab initio
Nuclides
' classification
Isotopes
– equal
Z
Isobars
– equal
A
Isotones
– equal
N
Isodiaphers
– equal
N
−
Z
Isomers
– equal all the above
Mirror nuclei
–
Z
↔
N
Stable
Magic
Even/odd
Halo
Borromean
Nuclear stability
Binding energy
p–n ratio
Drip line
Island of stability
Valley of stability
Stable nuclide
Radioactive decay
Alpha α
Beta β
2β
0v
β
+
K/L capture
Isomeric
Gamma γ
Internal conversion
Spontaneous fission
Cluster decay
Neutron emission
Proton emission
Decay energy
Decay chain
Decay product
Radiogenic nuclide
Nuclear fission
Spontaneous
Products
pair breaking
Photofission
Capturing processes
electron
2×
neutron
s
r
proton
p
rp
High-energy processes
Spallation
by cosmic ray
Photodisintegration
Nucleosynthesis
and
nuclear astrophysics
Nuclear fusion
Processes:
Stellar
Big Bang
Supernova
Nuclides:
Primordial
Cosmogenic
Artificial
High-energy nuclear physics
Quark–gluon plasma
RHIC
LHC
Scientists
Alvarez
Becquerel
Bethe
A. Bohr
N. Bohr
Chadwick
Cockcroft
Ir. Curie
Fr. Curie
Pi. Curie
Skłodowska-Curie
Davisson
Fermi
Hahn
Jensen
Lawrence
Mayer
Meitner
Oliphant
Oppenheimer
Proca
Purcell
Rabi
Rutherford
Soddy
Strassmann
Świątecki
Szilárd
Teller
Thomson
Walton
Wigner
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