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Nonelastic Breakup

Nuclear Reaction Dynamics

Explore the fascinating process of nuclear breakup and fragment absorption

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What is Nonelastic Breakup?

Nonelastic breakup is a nuclear reaction process in which a projectile nucleus breaks apart when interacting with a target nucleus, and some of the fragments interact with the target through nuclear forces rather than simply scattering elastically.

Approach

A loosely bound projectile (deuteron, 6Li, 7Li, 9Be, or halo nuclei) approaches the target

Dissociation

The projectile dissociates into its constituent clusters under Coulomb and nuclear forces

Fragment Reaction

At least one fragment undergoes nuclear reaction with target: absorption, fusion, or transfer

Key Characteristics

  • Partial Absorption - Not all fragments react with the target
  • Incomplete Fusion - Distinct from complete fusion of intact projectile
  • Complex Products - Multiple reaction products are generated

Elastic vs Nonelastic Breakup

Elastic Breakup

Coulomb Dissociation

Also known as diffractive breakup

  • All fragments scatter elastically
  • No nuclear reaction occurs
  • Fragments retain original properties
  • Both fragments escape the target
VS

Nonelastic Breakup

Fragment Absorption

Fragment interacts via nuclear forces

  • At least one fragment is absorbed
  • Fusion or transfer may occur
  • Produces incomplete fusion products
  • One fragment escapes as spectator

Typical Projectile Nuclei

Deuteron (d)

p + n

The simplest composite nucleus, consisting of one proton and one neutron loosely bound together. With a binding energy of only 2.22 MeV, it easily breaks up near a target nucleus.

Typical reactions:
d + A → p + (n + A) or d + A → n + (p + A)

Lithium-6 (6Li)

α + d

Can be viewed as an alpha particle + deuteron cluster structure. Breakup threshold energy is approximately 1.47 MeV.

Typical reaction:
6Li → α + d, with one fragment absorbed by target

Lithium-7 (7Li)

α + t

Alpha particle + triton cluster structure. Breakup threshold energy is approximately 2.47 MeV.

Typical reaction:
7Li → α + t, fragments may trigger secondary reactions

11Be - One-Neutron Halo Nucleus

10Be + n

A classic one-neutron halo nucleus with an extremely low neutron separation energy of only 0.50 MeV. The valence neutron extends far beyond the 10Be core, forming an extended halo structure.

Typical reaction:
11Be → 10Be + n, with the halo neutron easily stripped

11Li - Two-Neutron Halo Nucleus

9Li + n + n

A Borromean two-neutron halo nucleus. The two-neutron separation energy is only 0.37 MeV, while neither 10Li nor the dineutron is bound. All three components are needed for binding.

Typical reaction:
11Li → 9Li + 2n, exhibiting anomalously large reaction cross-section

Research Significance

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Fusion Studies

Understanding fusion mechanisms near the Coulomb barrier, distinguishing complete fusion from incomplete fusion

Radioactive Ion Beams

Production and study of exotic nuclei far from the stability line

Nuclear Astrophysics

Understanding reaction pathways in stellar nucleosynthesis processes

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Nuclear Structure

Probing cluster structures in weakly bound nuclei and halo nucleus properties

Key Physical Quantities

σtotal = σCF + σEB + σNEB

Total reaction cross-section components:
CF = Complete Fusion, EB = Elastic Breakup,
NEB = Nonelastic Breakup (includes Incomplete Fusion)

Eth = Sn or Sp

Breakup threshold energy equals the separation energy

Explore the NEB Comic

Discover nonelastic breakup through visual storytelling

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Simulation Controls

50 MeV
2.3 fm