light-mass nuclei combine to form a heavier, more stable nucleus
Front
nuclear fusion
Back
a nuclear reaction in which a positron is emitted
Front
positron decay
Back
unstable nuclei lose energy by emitting radiation
Front
radioactive decay
Back
Front
nuclear fission equation
Back
Front
Back
4/2 He
Front
alpha decay
Back
0/0 y
Front
gamma radiation symbol
Back
1/0+4/2 -> 1/1 + 4/2
Front
Transmutation equation
Back
1/1 -> 1/0 + 0/1 e
Front
Positron Decay/Emission
Back
electromagnetic radiation emitted during radioactive decay and having an extremely short wavelength
excited - > ground state
Front
gamma radiation
Back
alpha decay, gamma radiation, b-decay, positron decay, electron capture
Front
radioactive decay
Back
1/0 n -> 1/1P + 0/-1 e
Front
Beta decay equation:
Back
a heavy nucleus splits into two smaller nuclei of roughly equal mass
Front
nuclear fission
Back
1/1 P+ 0/-1 e - > 1/0n
Front
electron capture
Back
222/88 Ra ---> 4/2 He + 218/86 R
Front
alpha decay equation
Back
The process whereby a radioactive element releases energy slowly over a long period of time to lower its energy and become more stable is best described as
a. combustion
b. decay
c. fusion
d. fission
Front
B- decay
Back
an inner orbital electron is captured by the nucleus of its own atom
Front
electron capture
Back
Process of changing one element to another through radioactive decay
Front
Transmutation
Back
Front
nuclear fusion equation
Back
A nuclear reaction in which an atom emits an alpha particle consisting of two protons and two neutrons. This increases the atomic number by 2 and the mass number by 4.