42-5 Beta Decay#

Prompts

  • Write the beta-minus decay reaction at the nucleon level. What changes in the nucleus (\(Z\), \(N\), \(A\))? Why is an antineutrino required?

  • Beta-plus decay emits a positron. Write the reaction. How does it differ from beta-minus in terms of the nucleus and the neutrino?

  • What is electron capture? When might it compete with or replace beta-plus decay?

  • The beta particle (electron or positron) has a continuous energy spectrum, not a single value. Why? What would the spectrum look like without the neutrino?

  • How do you calculate the Q-value for beta-minus decay from atomic masses? Why must the daughter be heavier than the parent for beta-plus?

Lecture Notes#

Overview#

  • Beta decay changes a neutron into a proton (or vice versa) within the nucleus, keeping \(A\) constant but changing \(Z\). Three processes: beta-minus (\(n \to p\)), beta-plus (\(p \to n\)), and electron capture (\(p + e^- \to n\)).

  • A neutrino or antineutrino is emitted in each process. It is required for energy, momentum, and lepton number conservation — and it explains the continuous energy spectrum of the beta particle.

  • The Q-value determines whether a given beta decay is energetically allowed; mass tables (or atomic masses) are used to compute it.


Beta-Minus Decay (\(\beta^-\))#

In beta-minus decay, a neutron inside the nucleus converts to a proton, emitting an electron and an antineutrino:

(451)#\[ n \to p + e^- + \bar{\nu}_e \]

At the nuclear level: \(_Z^A\text{X} \to _{Z+1}^{A}\text{Y} + e^- + \bar{\nu}_e\). The mass number \(A\) is unchanged; the atomic number increases by 1. Example: \(^{14}\text{C} \to ^{14}\text{N} + e^- + \bar{\nu}_e\).


Beta-Plus Decay (\(\beta^+\))#

In beta-plus decay, a proton converts to a neutron, emitting a positron (\(e^+\)) and a neutrino:

(452)#\[ p \to n + e^+ + \nu_e \]

At the nuclear level: \(_Z^A\text{X} \to _{Z-1}^{A}\text{Y} + e^+ + \nu_e\). Example: \(^{11}\text{C} \to ^{11}\text{B} + e^+ + \nu_e\).

Energetic requirement

Beta-plus requires the parent to be heavier than the daughter by at least \(2m_e c^2\) (the rest energy of the created positron–electron pair). If the mass difference is too small, beta-plus is forbidden but electron capture may still occur.


Electron Capture (EC)#

In electron capture, a proton captures an atomic electron and converts to a neutron, emitting a neutrino:

(453)#\[ p + e^- \to n + \nu_e \]

At the nuclear level: \(_Z^A\text{X} + e^- \to _{Z-1}^{A}\text{Y} + \nu_e\). The captured electron usually comes from the innermost shell (K-shell); the process is sometimes written as K-capture.

Process

Nucleon change

Emitted

\(Z\) change

\(\beta^-\)

\(n \to p\)

\(e^-\), \(\bar{\nu}_e\)

\(+1\)

\(\beta^+\)

\(p \to n\)

\(e^+\), \(\nu_e\)

\(-1\)

EC

\(p + e^- \to n\)

\(\nu_e\)

\(-1\)


Why the Neutrino?#

The neutrino (\(\nu_e\)) and antineutrino (\(\bar{\nu}_e\)) are electrically neutral, nearly massless particles that carry energy, momentum, and lepton number.

Why they are required:

  1. Energy spectrum: Without a third particle, the electron (or positron) would have a unique energy (two-body final state). Experimentally, the beta particle has a continuous spectrum from 0 up to a maximum \(E_{\max} = Q\). The “missing” energy is carried by the neutrino.

  2. Momentum: A two-body decay would fix the electron’s momentum. The three-body decay allows a range of momentum sharing.

  3. Lepton number: The electron has lepton number \(L = +1\); the antineutrino has \(L = -1\). The decay \(n \to p + e^-\) would violate lepton number; adding \(\bar{\nu}_e\) conserves it.


Q-Value for Beta Decay#

The decay energy \(Q\) is the total kinetic energy shared by the products. For beta-minus (using atomic masses; the \(Z\) electrons cancel):

(454)#\[ Q_{\beta^-} = (M_{\text{parent}} - M_{\text{daughter}})c^2 \]

For beta-plus, the daughter has one fewer electron than the parent; creating the positron requires \(2m_e c^2\):

(455)#\[ Q_{\beta^+} = (M_{\text{parent}} - M_{\text{daughter}} - 2m_e)c^2 \]

For electron capture, the parent atom has one more electron than the daughter nucleus needs:

(456)#\[ Q_{\text{EC}} = (M_{\text{parent}} - M_{\text{daughter}})c^2 - E_B \]

where \(E_B\) is the binding energy of the captured electron (usually small compared to \(Q\)).


Summary#

  • \(\beta^-\): \(n \to p + e^- + \bar{\nu}_e\); \(Z \to Z+1\), \(A\) unchanged.

  • \(\beta^+\): \(p \to n + e^+ + \nu_e\); \(Z \to Z-1\).

  • EC: \(p + e^- \to n + \nu_e\); \(Z \to Z-1\); competes with \(\beta^+\) when \(Q_{\beta^+}\) is small.

  • Neutrino/antineutrino: conserves energy, momentum, lepton number; explains continuous beta spectrum.

  • \(Q > 0\) required for each process; use atomic masses with care for \(\beta^+\) and EC.