The Effect of Bound Dineutrons upon BBN
arXiv:astro-ph/0312388 · doi:10.1103/PhysRevD.70.043512
Abstract
We have examined the effects of a bound dineutron, n2, upon big bang nucleosynthesis (BBN) as a function of its binding energy B_n2. We find a weakly bound dineutron has little impact but as B_n2 increases its presence begins to alter the flow of free nucleons to helium-4. Due to this disruption, and in the absence of changes to other binding energies or fundamental constants, BBN sets a reliable upper limit of B_n2 <~ 2.5 MeV in order to maintain the agreement with the observations of the primordial helium-4 mass fraction and D/H abundance.
References in corpus (17)
- The cosmological baryon density from the deuterium to hydrogen ratio towards QSO absorption systems: D/H towards Q1243+3047
- Cosmological bounds on neutrino degeneracy improved by flavor oscillations
- Analytical treatment of neutrino asymmetry equilibration from flavour oscillations in the early universe
- Stringent Constraints on Cosmological Neutrino-Antineutrino Asymmetries from Synchronized Flavor Transformation
- Effective number of neutrinos and baryon asymmetry from BBN and WMAP
- The Quark-Mass Dependence of Two-Nucleon Systems
- Variation of Fundamental Couplings and Nuclear Forces
- An Infrared Renormalization Group Limit Cycle in QCD
- Does the fine-structure constant vary with cosmological epoch?
- Limits on Cosmological Variation of Strong Interaction and Quark Masses from Big Bang Nucleosynthesis, Cosmic, Laboratory and Oklo Data
- Hiding relativistic degrees of freedom in the early universe
- Primordial nucleosynthesis with a varying fine structure constant: An improved estimate
- Dependence of hadronic properties on Quark Masses and Constraints on their Cosmological Variation
- Big Bang nucleosynthesis and cosmic microwave background constraints on the time variation of the Higgs vacuum expectation value
- The Chemical Evolution of Mg Isotopes vs. the Time Variation of the Fine Structure Constant
- BBN And CMB Constraints On Dark Energy
- BBN and Lambda_QCD
Cited by in corpus (15)
- Primordial Nucleosynthesis: from precision cosmology to fundamental physics
- Coupled Variations of Fundamental Couplings and Primordial Nucleosynthesis
- Life at the Interface of Particle Physics and String Theory
- Primordial nucleosynthesis as a probe of fundamental physics parameters
- Nuclear matrix elements from lattice QCD for electroweak and beyond-Standard-Model processes
- The variation of fundamental constants and the role of A=5 and A=8 nuclei on primordial nucleosynthesis
- Nuclear Astrophysics of Worlds in the String Landscape
- -dependence of light nuclei and nucleosynthesis
- Constraints on a possible dineutron state from pionless EFT
- On the Quark Mass Dependence of Two Nucleon Observables
- Search for a bound di-neutron by comparing He(e,e'p)d and H(e,e'p)X measurements
- Effects of Bound Diprotons and Enhanced Nuclear Reaction Rates on Stellar Evolution
- Impact of dineutrons on nuclear compositions of a core-collapse supernova
- Light Neutral Clusters in Supernova Matter
- Experimental Evidence of a Bonded Dineutron Existence