Section 1

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light-mass nuclei combine to form a heavier, more stable nucleus

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Date created

Mar 14, 2020

Cards (20)

Section 1

(20 cards)

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.

Front

alpha decay

Back