2013
DOI: 10.1103/physrevd.87.123530
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Mirror matter can alleviate the cosmological lithium problem

Abstract: The abundance of lithium-7 confronts cosmology with a long lasting problem between the predictions of standard big bang nucleosynthesis and the baryonic density determined from the cosmic microwave background observations. This article investigates the influence of the existence of a mirror world, focusing on models in which neutrons can oscillate into mirror neutrons. Such a mechanism allows for an effective late time neutron injection, which induces an increase of the destruction of beryllium-7, due to an in… Show more

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Cited by 29 publications
(44 citation statements)
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“…1 It is of key importance that in nuclei n → n transition is forbidden by energy conservation and thus nuclear stability bounds give no limitations on τ , while for free neutrons n-n oscillation is affected by magnetic fields and coherent interactions with matter which makes this phenomenon rather elusive [15,16]. On the other hand, it is striking that n → n transitions faster than the neutron decay can have far going implications for the propagation of ultra-high energy cosmic rays at cosmological distances [19], for the neutrons from solar flares [20], for primordial nucleosynthesis [21] and for neutron stars [22]. 2 The possibility of fast n−n oscillations can be tested in experiments searching for neutron disappearance n → n and regeneration n → n → n [15] as well as via nonlinear effects on the neutron spin precession [16].…”
Section: Introductionmentioning
confidence: 99%
“…1 It is of key importance that in nuclei n → n transition is forbidden by energy conservation and thus nuclear stability bounds give no limitations on τ , while for free neutrons n-n oscillation is affected by magnetic fields and coherent interactions with matter which makes this phenomenon rather elusive [15,16]. On the other hand, it is striking that n → n transitions faster than the neutron decay can have far going implications for the propagation of ultra-high energy cosmic rays at cosmological distances [19], for the neutrons from solar flares [20], for primordial nucleosynthesis [21] and for neutron stars [22]. 2 The possibility of fast n−n oscillations can be tested in experiments searching for neutron disappearance n → n and regeneration n → n → n [15] as well as via nonlinear effects on the neutron spin precession [16].…”
Section: Introductionmentioning
confidence: 99%
“…27 Modern determinations based on radar ranging led to 28 43.2 ± 0.9 " cy −1 . The latest determination, based on optical data, yields 29 cleosynthesis, 43,44 gravitational microlensing, 45,46 anisotropies 47 in the Cosmic Microwave Background (CMB), Baryon Acoustic Oscillation (BAO) clustering in sky surveys, 48 and structure formation 49,50 elucidated that galactic and extragalactic obscure mass cannot be made, to a large extent, of particles of ordinary matter. This is what is commonly meant today by the denomination 'Dark Matter'.…”
Section: Introductionmentioning
confidence: 99%
“…[49] and references therein). Other non-standard solutions to the lithium problem include photon cooling by axions [50] or extra neutrons from a mirror world [51].…”
Section: Non Standard Big-bang Nucleosynthesismentioning
confidence: 99%