Possible explanation of primordial ⁷Li deficit
Pith reviewed 2026-06-28 09:00 UTC · model grok-4.3
The pith
Primordial black holes supply neutrons that convert excess ^7Li into helium nuclei.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
A reduction mechanism of the theoretically predicted excessive abundance of ^7Li via baryons evaporated by primordial black holes is suggested. It is shown that the fraction of ^7Li with respect to the number density of baryons can be diminished down to the observed value via the process of ^7Li transformation by neutron capture. The created in this process ^8Li or ^8Be quickly decay into a pair of ^4He nuclei.
What carries the argument
Neutron capture on ^7Li nuclei supplied by baryons evaporated from primordial black holes, followed by decay of the product into ^4He pairs.
If this is right
- The lithium problem can be resolved without changes to standard big bang nucleosynthesis calculations.
- The ^7Li reduction occurs through a specific decay chain that produces only helium and no other light elements in comparable quantities.
- The required neutron supply depends on the abundance and evaporation timing of primordial black holes.
- Other primordial abundances stay consistent with standard predictions.
- The mechanism operates after the main phase of big bang nucleosynthesis but before significant stellar processing.
Where Pith is reading between the lines
- This would impose new upper and lower bounds on the density of primordial black holes in a narrow mass range.
- The same neutron flux might produce small shifts in deuterium or helium-3 that could be searched for in high-precision observations.
- If confirmed, the model links the lithium problem directly to possible early-universe sources of dark matter or gravitational-wave backgrounds.
- The process could be tested by comparing lithium abundances in regions with different inferred early neutron densities, such as near ancient black hole remnants.
Load-bearing premise
Primordial black holes must exist in sufficient numbers and evaporate at the correct epoch to supply the necessary neutrons for the capture process without violating other cosmological constraints.
What would settle it
Observation of a ^7Li abundance that remains high even in regions where neutron fluxes from evaporating black holes would have been present, or direct evidence ruling out the required population of evaporating primordial black holes at the relevant masses and times.
Figures
read the original abstract
A reduction mechanism of the theoretically predicted excessive abundance of $^7$Li via baryons evaporated by primordial black holes is suggested. It is shown that the fraction of $^7$Li with respect to the number density of baryons can be diminished down to the observed value via the process of $^7$Li transformation by neutron capture. The created in this process $^8$Li or $^8$Be quickly decay into a pair of $^4$He nuclei.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript proposes that evaporation of primordial black holes supplies neutrons which capture on ^7Li, converting it to ^8Li or ^8Be that subsequently decay into ^4He pairs, thereby reducing the primordial ^7Li-to-baryon ratio from its standard BBN prediction down to the observed value.
Significance. If quantitatively demonstrated with viable PBH parameters, the mechanism would constitute a novel post-BBN processing channel capable of resolving the lithium problem while preserving other light-element abundances. The current text, however, contains no derivation or numerical evaluation, so the significance cannot be assessed.
major comments (2)
- [Abstract] Abstract: the statement 'it is shown that the fraction of ^7Li ... can be diminished down to the observed value' is unsupported; no neutron-capture rate equations, fluence calculation, or mapping from PBH mass function and evaporation epoch to the required neutron density appear anywhere in the manuscript.
- [Abstract] Abstract: the proposal inherits all standard PBH constraints (gamma-ray backgrounds, CMB spectral distortions, and modifications to η and other BBN yields from injected baryons) yet provides no check that the required PBH abundance and mass range remain consistent with those bounds.
Simulated Author's Rebuttal
We thank the referee for the careful reading of our manuscript and the constructive comments. The report correctly identifies that the current text is a concise proposal without quantitative derivations. We respond to each major comment below.
read point-by-point responses
-
Referee: [Abstract] Abstract: the statement 'it is shown that the fraction of ^7Li ... can be diminished down to the observed value' is unsupported; no neutron-capture rate equations, fluence calculation, or mapping from PBH mass function and evaporation epoch to the required neutron density appear anywhere in the manuscript.
Authors: We agree that the wording 'it is shown' is too definitive for a short conceptual note that contains no rate equations or fluence calculations. The manuscript presents a possible mechanism rather than a completed demonstration. We will revise the abstract to replace 'it is shown' with 'we suggest' or 'we propose', and we will add a brief order-of-magnitude estimate of the required neutron fluence in the main text to support the claim at a qualitative level. revision: partial
-
Referee: [Abstract] Abstract: the proposal inherits all standard PBH constraints (gamma-ray backgrounds, CMB spectral distortions, and modifications to η and other BBN yields from injected baryons) yet provides no check that the required PBH abundance and mass range remain consistent with those bounds.
Authors: The referee is correct that consistency with existing PBH bounds must be verified for any concrete parameter choice. The present manuscript does not perform these checks, as its scope is limited to identifying the lithium-reduction channel. In revision we will insert a short paragraph that references the principal constraints (gamma-ray backgrounds, CMB distortions, and BBN yield modifications) and states that the required PBH mass and abundance lie in a window that appears marginally allowed, while noting that a full scan is left for future work. revision: yes
Circularity Check
No circularity: mechanism is a proposed physical process relying on external PBH neutron injection, with no equations, fits, or self-citations reducing claims to inputs by construction.
full rationale
The abstract and available text describe a suggested reduction of ^7Li via neutron capture from PBH evaporation, leading to ^8Li/^8Be decay into ^4He. No derivation chain, equations, or parameters are shown that would qualify as self-definitional, fitted-input predictions, or load-bearing self-citations. The central claim is a qualitative mechanism whose viability depends on unexamined external constraints (PBH abundance, timing, and consistency with BBN/eta), but the paper does not present any step that reduces by construction to its own inputs. This is the normal case of a self-contained suggestion without circular structure.
Axiom & Free-Parameter Ledger
Reference graph
Works this paper leans on
-
[1]
S. Navaset al.[Particle Data Group], “Review of particle physics,” Phys. Rev. D110 (2024) no.3, 030001. doi:10.1103/PhysRevD.110.030001
-
[2]
Planck 2018 results. VI. Cosmological parameters
N. Aghanimet al.[Planck], “Planck 2018 results. VI. Cosmological parameters,” Astron. Astrophys.641(2020), A6 [erratum: Astron. Astrophys.652(2021), C4] doi:10.1051/0004-6361/201833910 [arXiv:1807.06209 [astro-ph.CO]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1051/0004-6361/201833910 2018
-
[3]
Re-examining the Lithium abun- dance problem in Big-Bang nucleosynthesis,
V. Singh, D. Bhowmick and D. N. Basu, “Re-examining the Lithium abun- dance problem in Big-Bang nucleosynthesis,” Astropart. Phys.162(2024), 102995 doi:10.1016/j.astropartphys.2024.102995 [arXiv:2304.08032 [nucl-th]]. 9
-
[4]
S. W. Hawking, “Black hole explosions,” Nature248(1974), 30-31. doi:10.1038/248030a0
-
[5]
Particle Emission Rates from a Black Hole: Massless Particles from an Uncharged, Nonrotating Hole
D. N. Page, “Particle Emission Rates from a Black Hole: Massless Parti- cles from an Uncharged, Nonrotating Hole,” Phys. Rev. D13(1976), 198-206 doi:10.1103/PhysRevD.13.198
-
[6]
Recombination of hydrogen in the hot model of the universe,
Y. B. Zeldovich, V. G. Kurt and R. A. Sunyaev, “Recombination of hydrogen in the hot model of the universe,” Zh. Eksp. Teor. Fiz.55(1968), 278-286 (Sov.Phys.JETP 28(1969) 146). 46 (1969)
1968
-
[7]
Calculation of anti-proton annihilation on helium nuclei,
A. A. Sibirtsev, “Calculation of anti-proton annihilation on helium nuclei,” Sov. J. Nucl. Phys.55(1992), 541-546
1992
-
[8]
Antiproton annihilation on light nuclei at very low energies
K. V. Protasov, G. Bonomi, E. Lodi Rizzini and A. Zenoni, “Anti-proton annihi- lation on light nuclei at very low- energies,” Eur. Phys. J. A7(2000), 429-434. doi:10.1007/s100500050413 [arXiv:nucl-th/9911005 [nucl-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1007/s100500050413 2000
-
[9]
Low-energy Antiproton Interaction with Helium
W. R. Gibbs, “Low-energy anti-proton interaction with helium,” Phys. Rev. A56 (1997), 3553 doi:10.1103/PhysRevA.56.3553 [arXiv:nucl-th/9705007 [nucl-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physreva.56.3553 1997
-
[10]
Measuring theα- particle charge radius with muonic helium-4 ions,
J. J. Krauth, K. Schuhmann, M. A. Ahmed, F. D. Amaro, P. Amaro, F. Biraben, T. L. Chen, D. S. Covita, A. J. Dax and M. Diepold,et al.“Measuring theα- particle charge radius with muonic helium-4 ions,” Nature589(2021) no.7843, 527-531 doi:10.1038/s41586-021-03183-1
-
[11]
H. Yanagisawa, M. Ouchi, A. Matsumoto, M. Kawasaki, K. Murai, K. Nakajima, K. Kohri, Y. Sugahara, K. Nagamine and I. Tanaka,et al.“EMPRESS. XV. A New Determination of the Primordial Helium Abundance Suggesting a Moderately LowY P Value,” [arXiv:2506.24050 [astro-ph.GA]]
-
[12]
P. A. Kislitsyn, S. A. Balashev, M. T. Murphy, C. Ledoux, P. Noterdaeme and A. V. Ivanchik, “A new precise determination of the primordial abundance of deu- terium: measurement in the metal-poor sub-DLA system at z = 3.42 towards quasar J 1332+0052,” Mon. Not. Roy. Astron. Soc.528(2024) no.3, 4068-4081 doi:10.1093/mnras/stae248 [arXiv:2401.12797 [astro-ph.CO]]
-
[13]
The radiative neutron capture on 2H, 6Li, 7Li, 12C and 13C at astrophysical energies
S. B. Dubovichenko, A. V. Dzhazairov-Kakhramanov and N. A. Burkova, “The ra- diative neutron capture on 2H, 6Li, 7Li, 12C and 13C at astrophysical energies,” Int. J. Mod. Phys. E22(2013), 1350028 doi:10.1142/S0218301313500286 [arXiv:1209.1702 [nucl-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1142/s0218301313500286 2013
-
[14]
Neutron capture gamma rays from Lithium, Boron, and Nitrogen
A. Bartholomew and P. J. Campion, “Neutron capture gamma rays from Lithium, Boron, and Nitrogen”, Can. J. Phys.35(1975) 1347
1975
-
[15]
(n,γ)-Spektren und Wirkungsquerschnitte von Lithium,. Beryllium und Kohlenstoff
L. Jarczyk, et al., “(n,γ)-Spektren und Wirkungsquerschnitte von Lithium,. Beryllium und Kohlenstoff”, Helv. Phys. Acta34(1961) 483. 10
1961
-
[16]
Thermal capture cross sections for 6Li and 7Li
E. T. Jurney, “Thermal capture cross sections for 6Li and 7Li”, U.S. Nucl. Data Comm.9(1973) 109
1973
-
[17]
Determination of thermal neu- tron radiative capture cross section of? 6Li
Chang Su Park, Gwang Min Sun and H. D. Choi, “Determination of thermal neu- tron radiative capture cross section of? 6Li”, Nucl. Instr. Meth.B 245(2006) 367. https://doi.org/10.1016/j.nimb.2005.11.166
-
[18]
H. Atek, I. Labbe, L.J. Furtaket al, ”Most of the photons that reion- ized the Universe came from dwarf galaxies”, Nature626(2024) 975-978. https://doi.org/10.1038/s41586-024-07043-6 11
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.