What is the neutron number of mercury?
8
80
201
121
201-80=121
What is the definition of an isotope?
a) Same proton number so same element, but different number of neutrons
b) Same mass number but different atomic number
c) Same number of neutrons but different number of protons
d) the same number of protons and neutrons but they have different amounts of energy.
A
Which force is responsible for the transformation of a neutron in to a proton?
Nuclear force
Strong force
Weak force
Electromagnetic force
weak
How many electrons are in the M shell?
25
16
18
36
ans: 18
m is the third shell
3 squared = 9
x2= 18
2(n^2)
Using the diagram, how much energy is released when an electron moves from L–>K?
11eV
69eV
2.8eV
58eV
the difference between the two shells
58eV
what is an isobar
equal A. Same mass number but different atomic number
what is an isotone
same N
Same number of neutrons but different number of protons
what is an isomer
In atomic physics they have the same number of protons and neutrons but they have different amounts of energy. They are in a metastable state.
nucleons and the nucleus are held together by which force?
strong force
which radioactive decay modes are isobaric?
the mass stays the same: isomeric transition, positron emission (peta positive), beta negative, electron capture.
which radioactive decay types cause transmutation
a different element is formed: alpha decay, beta neg, beta positive, electron capture (spontaneous fission)
below a z number of 20, what is the stable ratio of protons and neutrons?
1:1
above a z number of 20, what is a stable ratio of neutrons to protons?
1.5:1
what is the equation for negatron decay/ beta minus decay? when does it occur?
too many neutrons
what is the equation for alpha decay? when does it occur?
too many nucleons- very heavy, mass over 200
what is the equation for electron capture? when does it occur?
p+e-= Neutron and antineutrino. when too few neutrons
This competes with β+ decay as it also occurs in proton-rich nuclei. If the energy difference between the parent and daughter nuclides is too low for positron emission an inner shell electron is captured by the nucleus converting a proton into a neutron (i.e. positive + negative = neutral). As with β+ decay the mass number remains the same but the atomic number decreases by 1. This emission causes characteristic X-rays.
what is the equation for beta positive decay? when does it occur?
too few neutrons. The extra proton decays into a neutron (which is retained in the nucleus), a positron (β+ or e) and an electron neutrino (ve). A neutron is gained, and a proton is lost meaning the mass number remains equal but the atomic number decreases by 1. This form of radioactivity, with the production of a positron, is important in PET imaging. The emitted positron travels only a minimal distance before it undergoes an annihilation reaction with the production of two 0.511 MeV photons that travel in opposite directions to one another.
what is isomeric transition? when does it occur?
A radionuclide in a metastable excited state decays to its ground state by isomeric transition and the number of protons and neutrons remain the same and the mass number and atomic number remain unchanged. Excess energy is emitted as gamma ray, internal conversion electron or both. Internal conversion is energy transfer to an orbital electron ejecting it. The ejected electron is called a conversion electron (E = gamma ray - binding E), often causes characteristic XR or Auger electron. e.g. technectium
which decay produces gamma radiation?
isomeric transition
The ratio of protons and neutrons should mean it is stable, but it is still not in a resting state, the excess energy is given off by isomeric transition. A gamma ray is emitted. Or the nucleus undergoes internal conversion (the de- excitation energy is transferred to a K, L or M shell electron, the electron is ejected and has the kinetic energy equal to that of the gamma ray minus the electron binding energy. The vacancy created is filled by an electron cascade as previously described) .The mass number and atomic number remain unchanged.- gamma emission.
e.g. Tc-99m → Tc-99 + 140 keV γ rays
A. High energy photons
B. Heavy particles with a short range
C. Light particles that can be subdivided into β+ and β-
D. Electrically neutral particles with little mass
B
A. Helium atom
B. Positron
C. Electron and electron antineutrino
D. Characteristic X-rays
C
A. Alpha decay
B. Electron capture
C. Isomeric transition
D. Negatron decay
B
A. Alpha particles
B. Helium atom
C. Gamma rays or internal conversion electrons
D. Positrons and neutrinos
C
A. Characteristic X-rays
B. Auger electrons
C. Two 0.511 MeV photons
D. A helium nucleus
C