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Nuclear Physics Formulas

Complete collection of nuclear physics formulas with detailed explanations.

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Nuclear Decay

Radioactive Decay

N(t)=N0e−λtN(t) = N_0 e^{-\lambda t}

Number of nuclei at time t equals initial number times exponential of negative decay constant times time.

Notation:

N(t):Number of nuclei at time t
N₀:Initial number of nuclei
λ:Decay constant
t:Time

Units:

N(t), N₀:dimensionless
λ:s⁻¹
t:s

Applications:

  • •Carbon dating
  • •Nuclear medicine
  • •Radiation safety

Limitations:

Exponential decay

Half-Life

T1/2=ln⁡(2)λT_{1/2} = \frac{\ln(2)}{\lambda}

Half-life equals natural logarithm of 2 divided by decay constant.

Notation:

T₁/₂:Half-life
λ:Decay constant

Units:

T₁/₂:s
λ:s⁻¹

Applications:

  • •Nuclear dating
  • •Medical isotopes
  • •Nuclear waste

Limitations:

First-order decay

Decay Rate

A=λNA = \lambda N

Activity equals decay constant times number of nuclei.

Notation:

A:Activity
λ:Decay constant
N:Number of nuclei

Units:

A:Bq (becquerels)
λ:s⁻¹
N:dimensionless

Applications:

  • •Radiation measurement
  • •Nuclear power
  • •Medical imaging

Limitations:

First-order decay

Mean Lifetime

τ=1λ\tau = \frac{1}{\lambda}

Mean lifetime equals reciprocal of decay constant.

Notation:

τ:Mean lifetime
λ:Decay constant

Units:

τ:s
λ:s⁻¹

Applications:

  • •Nuclear stability
  • •Decay calculations
  • •Particle physics

Limitations:

Exponential decay

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Nuclear Reactions

Mass-Energy Equivalence

E=mc2E = mc^2

Energy equals mass times speed of light squared.

Notation:

E:Energy
m:Mass
c:Speed of light

Units:

E:J
m:kg
c:3 × 10⁸ m/s

Applications:

  • •Nuclear fusion
  • •Nuclear fission
  • •Particle physics

Limitations:

Rest mass energy

Binding Energy

Eb=Δmc2E_b = \Delta mc^2

Binding energy equals mass defect times speed of light squared.

Notation:

E_b:Binding energy
Δm:Mass defect
c:Speed of light

Units:

E_b:J
Δm:kg
c:3 × 10⁸ m/s

Applications:

  • •Nuclear stability
  • •Fusion reactions
  • •Nuclear power

Limitations:

Rest mass approximation

Q-Value

Q=(minitial−mfinal)c2Q = (m_{initial} - m_{final})c^2

Q-value equals initial mass minus final mass times speed of light squared.

Notation:

Q:Q-value
m_initial:Initial mass
m_final:Final mass
c:Speed of light

Units:

Q:J
m_initial, m_final:kg
c:3 × 10⁸ m/s

Applications:

  • •Nuclear reactions
  • •Energy release
  • •Reaction feasibility

Limitations:

Rest mass approximation

Nuclear Cross Section

σ=RΦn\sigma = \frac{R}{\Phi n}

Cross section equals reaction rate divided by flux times target density.

Notation:

σ:Cross section
R:Reaction rate
Φ:Particle flux
n:Target density

Units:

σ:barn (10⁻²⁸ m²)
R:s⁻¹
Φ:m⁻²s⁻¹
n:m⁻³

Applications:

  • •Nuclear scattering
  • •Reaction rates
  • •Neutron physics

Limitations:

Point-like particles

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Fission and Fusion

Fission Energy

Efission=(mU−mfragments)c2E_{fission} = (m_U - m_{fragments})c^2

Fission energy equals uranium mass minus fragment masses times speed of light squared.

Notation:

E_fission:Fission energy
m_U:Uranium mass
m_fragments:Fragment masses
c:Speed of light

Units:

E_fission:J
m_U, m_fragments:kg
c:3 × 10⁸ m/s

Applications:

  • •Nuclear power plants
  • •Atomic bombs
  • •Energy production

Limitations:

Rest mass approximation

Fusion Energy

Efusion=(mreactants−mproducts)c2E_{fusion} = (m_{reactants} - m_{products})c^2

Fusion energy equals reactant masses minus product masses times speed of light squared.

Notation:

E_fusion:Fusion energy
m_reactants:Reactant masses
m_products:Product masses
c:Speed of light

Units:

E_fusion:J
m_reactants, m_products:kg
c:3 × 10⁸ m/s

Applications:

  • •Hydrogen bombs
  • •Fusion reactors
  • •Stellar energy

Limitations:

Rest mass approximation

Critical Mass

Mcritical=π2D2νΣfM_{critical} = \frac{\pi^2 D^2}{\nu\Sigma_f}

Critical mass equals π squared times diffusion coefficient squared divided by neutron velocity times fission cross section.

Notation:

M_critical:Critical mass
D:Diffusion coefficient
ν:Neutron velocity
Σ_f:Fission cross section

Units:

M_critical:kg
D:m
ν:m/s
Σ_f:m⁻¹

Applications:

  • •Nuclear weapons
  • •Reactor design
  • •Criticality safety

Limitations:

Spherical geometry

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Radiation Protection

Dose Rate

D˙=AΓd2\dot{D} = \frac{A\Gamma}{d^2}

Dose rate equals activity times gamma constant divided by distance squared.

Notation:

Ḋ:Dose rate
A:Activity
Γ:Gamma constant
d:Distance

Units:

Ḋ:Gy/h
A:Bq
Γ:Gy·m²/(h·Bq)
d:m

Applications:

  • •Radiation safety
  • •Shielding design
  • •Dose calculations

Limitations:

Point source

Half-Value Layer

HVL=ln⁡(2)μHVL = \frac{\ln(2)}{\mu}

Half-value layer equals natural logarithm of 2 divided by linear attenuation coefficient.

Notation:

HVL:Half-value layer
μ:Linear attenuation coefficient

Units:

HVL:m
μ:m⁻¹

Applications:

  • •Shielding design
  • •Radiation protection
  • •Material selection

Limitations:

Narrow beam geometry

Exposure Rate

X˙=AΓd2\dot{X} = \frac{A\Gamma}{d^2}

Exposure rate equals activity times gamma constant divided by distance squared.

Notation:

Ẋ:Exposure rate
A:Activity
Γ:Gamma constant
d:Distance

Units:

Ẋ:R/h
A:Ci
Γ:R·m²/(h·Ci)
d:m

Applications:

  • •Radiation monitoring
  • •Safety assessments
  • •Regulatory compliance

Limitations:

Point source