{"id":"26508f79-3177-4a48-b6a7-be6fdf567648","arxiv_id":"hep-ph/0312335","paper_version":1,"verdict":"CONDITIONAL","confidence":"MODERATE","novelty_score":3.0,"correctness_risk":"medium","formal_verification":"none","parameter_count":0,"one_line_summary":"A colder mirror sector with identical microphysics should generate a larger baryon asymmetry than ours, so mirror baryons can naturally account for the dark matter density.","lead":"This review argues that a hidden mirror sector with the same particle physics as ours, but colder, would produce a larger baryon asymmetry than our sector and could supply the dark matter. It is a compact entry point to a two-sector cosmology program that ties the visible-to-dark density coincidence to baryogenesis.","discovery_kind":"review","skeptic_critique":{"model":"selfhosted/deepseek-v4.1-flash","headline":"Eqs. (49)-(50) are internally inconsistent: the source term in Eq. (49) uses the mirror equilibrium density n'_eq^2, but the text's own physical picture (ordinary particles scattering into the mirror) requires n_eq^2; the two choices give beta differing by x^6, which for x = 0.3 is a factor of ~37.","rationale":"The reader's weakest_assumption correctly identifies the bookkeeping between B-L densities and physical baryon densities as the load-bearing soft spot, and the numerical stakes (a factor of ~37 for x = 0.3) are real. My analysis sharpens the diagnosis: the inconsistency is not that Eq. (50) drops an x^3 relative to Eq. (37), but that Eq. (49)'s source term uses the mirror equilibrium density n'_eq^2 while the text's own physical picture (ordinary particles scattering into the mirror) requires n_eq^2. With the physical source and ordinary-entropy normalization, Eq. (50) is correct and the qualitative claim survives; with Eq. (49) as printed, beta is x^6-suppressed and the claim fails. The paper never states which entropy normalization it uses for (B-L)', so the reader cannot tell which bookkeeping is intended. This is a fixable derivation error, not a refutation of the program, so CONDITIONAL is the right verdict. The reader's secondary concern (k = 1.5 is tuned to reproduce beta ~ 5) is softer: Eq. (45) does give independent parametric motivation for k ~ 1, and the paper is candid that it is a review. The D(k) form is quoted from ref. 29 (in preparation) but Eqs. (47)-(48) give the explicit closed form, so it is checkable; the CMB/LSS exclusions are deferred to ref. 31, which is a companion preprint, not a gap in the central argument. The qualitative chain (BBN bound x < 0.64, colder sector freezes out earlier, mirror asymmetry less damped) is coherent and the BBN arithmetic in Sect. 3 is correct. The single concrete check above would settle whether the numerical headline stands or falls.","tokens_in":28761,"tokens_out":13508,"duration_ms":259131,"concrete_test":"Re-derive Eq. (49) from the Boltzmann equation for l phi <-> l' phi', keeping the production term proportional to n_l n_phi (ordinary densities) and the back-reaction proportional to n'_{l'} n'_{phi'} (mirror densities). Check explicitly whether the source is n_eq^2 or n'_eq^2. Then recompute beta = n'_b/n_b with the corrected equation and with (B-L)' normalized by s (ordinary entropy) and by s' (mirror entropy) separately. If the physical source n_eq^2 gives beta = D(kx^3)/D(k) ~ 5 at k = 1.5, the central claim survives and Eq. (49) needs only a typo fix; if the literal Eq. (49) source n'_eq^2 is what the authors intend, beta is x^6-suppressed and the claim beta ~ 5 fails.","verdict_should_be":"CONDITIONAL","load_bearing_attack":"The reader is right that the bookkeeping around Eqs. (49)-(50) does not close, but the diagnosis can be sharpened. The text states (Sect. 4.3, just before Eq. 49) that 'the only relevant reactions are the ones with ordinary particles in the initial state.' For l phi -> l' phi', the production rate per unit volume is n_l n_phi <sigma v> ~ n_eq^2 <sigma v>, i.e. the source is set by the ordinary equilibrium density. The back-reaction l' phi' -> l phi is set by n'_eq^2 ~ x^6 n_eq^2, and the paper correctly encodes this in Gamma' = x^3 Gamma. So the Boltzmann equation for n'_{B-L} should read dn'/dt + 3Hn' + Gamma' n' = (3/4) Delta sigma n_eq^2, not (3/4) Delta sigma' n'_eq^2 as written in Eq. (49). With the corrected source, and normalizing (B-L)' by the ordinary entropy s (the convention that makes the paper's claim '(B-L)' = (B-L)_0 D(kx^3)' true), one obtains beta = n'_b/n_b = D(kx^3)/D(k), which is Eq. (50). With Eq. (49) as literally written (source n'_eq^2), one instead gets beta ~ x^6 D(kx^3)/D(k), which for x = 0.3 is ~0.135 rather than ~5. The paper's claimed (B-L)' = (B-L)_0 D(kx^3) is therefore consistent with the physical source but not with Eq. (49) as printed, and the normalization convention (s vs s') used for (B-L)' is never stated. This is a genuine internal inconsistency in the derivation of the central numerical claim, not merely a missing x^3 in Eq. (50).","agreement_with_reader":"agree"},"referee_report":{"model":"selfhosted/deepseek-v4.1-flash","summary":"This review develops the cosmology of a mirror sector that duplicates the Standard Model and communicates with it only gravitationally or through very weak messengers. The BBN bound on extra relativistic species requires the mirror temperature to be lower, T' = xT with x < 0.64 (Eq. 35). The paper argues that because the mirror sector is cooler, its baryogenesis freezes out earlier, and in GUT baryogenesis (§4.2) and in leptogenesis via ordinary-mirror scattering (§4.3) the mirror world acquires a larger baryon asymmetry per entropy, B' > B. It then proposes that mirror baryons constitute the dark matter, with Omega'_b/Omega_b = beta ≈ 1/D(k) (Eq. 50), reaching beta ≈ 5 for k ≈ 1.5, and discusses the consequences for mirror recombination, the mirror Jeans and Silk scales, the CMB and LSS power spectra (Figs. 4-5), and gravitational microlensing by mirror stars.","tokens_in":29140,"tokens_out":9978,"duration_ms":171736,"significance":"If the central argument holds, the paper offers a rare framework in which the visible and dark matter densities share a common origin and their near equality is not accidental. The BBN constraint is standard and correctly applied, and the parametric GUT-baryogenesis argument (k' = kx^2, D decreasing, hence B' > B) is internally coherent. The scenario makes falsifiable predictions — a damping of small-scale power for x > 0.3 in the pure MBDM case, and a microlensing mass scale near 0.5 M_sun — which is a genuine strength. The main reservation is that the quantitative dark-matter fraction rests on a derivation whose bookkeeping is not closed as printed.","major_comments":[{"comment":"The Boltzmann equation for n'_{B-L} as printed has the source term (3/4) Delta sigma' n'^2_eq, but the physical picture stated immediately above — 'the only relevant reactions are the ones with ordinary particles in the initial state' — requires the source to be (3/4) Delta sigma' n^2_eq. Since n'_eq = x^3 n_eq, the printed source suppresses the produced asymmetry by x^6; for x = 0.3 this is a factor of about 7e-4, which would give beta of order 10^-3 rather than the claimed ~5. The stated result (B-L)' = (B-L)_0 D(kx^3) is consistent only with the ordinary-density source. In addition, (B-L)' must be defined as n'_{B-L}/s (ordinary entropy), not n'_{B-L}/s'; with the latter convention beta acquires an extra x^3 and Eq. (50) becomes beta = x^3 D(kx^3)/D(k), which for x = 0.3 gives beta ≈ 0.14. The paper never states which convention it uses. Because Eq. (50) is the source of the headline beta ≈ 5 at k = 1.5, the source term must be corrected and the normalization convention stated explicitly. If the correct form appears in refs. 12-13, the review should not reproduce it incorrectly.","section":"§4.3, Eqs. (49)-(50)","authors_acknowledge":null,"authors_acknowledge_p":null},{"comment":"The statement that 'x is the only free parameter in our model' is not correct as applied to the dark-matter fraction. Eq. (50) gives beta ≈ 1/D(k), so beta depends on k, and the value beta ≈ 5 requires k ≈ 1.5. The 'natural' explanation of Omega_d ≈ 5 Omega_b therefore requires an additional order-unity condition on k that is neither derived nor argued to be generic in the leptogenesis parameter space. The paper should state what fixes k, whether k ~ 1.5 is typical, and soften the word 'naturally' in abstract:s4 accordingly.","section":"§3 (after Eq. 34) and §4.3, Eq. (50)","authors_acknowledge":null,"authors_acknowledge_p":null}],"minor_comments":[{"comment":"The mirror reaction rate scales as kx^2 in the GUT case and as kx^3 in the exchange case. A sentence explaining that this reflects the different temperature dependence of a decay rate versus a 2-to-2 scattering rate would let the reader see that the difference is physical rather than an inconsistency between the two sections.","section":"§4.2, Eq. (37) vs §4.3, Eq. (50)","authors_acknowledge":null,"authors_acknowledge_p":null},{"comment":"The claim that 'the baryon asymmetry in the mirror world should be larger' is true for B' = n'_B/s', but the dark-matter fraction involves x^3 B'/B (Eq. 37). The abstract should distinguish the per-entropy asymmetry from the density ratio, since only the latter bears on the dark-matter claim.","section":"Abstract (s3) and §4.2","authors_acknowledge":null,"authors_acknowledge_p":null},{"comment":"The depletion factor D(k), which sets the central number beta ≈ 5, is quoted from ref. 29, listed as 'in preparation'. A short derivation from Eq. (43) or an updated reference would let the reader check the functional form.","section":"Eqs. (47)-(48)","authors_acknowledge":null,"authors_acknowledge_p":null},{"comment":"The quantitative CMB/LSS constraints (x > 0.3 excluded for pure MBDM, x > 0.5 for the mixed case) are delegated to ref. 31. The text should state the cosmological parameters used and whether the mirror baryon acoustic oscillations are included in the plotted curves.","section":"§5, Figs. 4-5","authors_acknowledge":null,"authors_acknowledge_p":null},{"comment":"The BBN bound epsilon < 3e-8 on the photon kinetic mixing is quoted without derivation. A sentence on how it follows from e+e- -> e'+e'- energy transfer would be useful.","section":"§2.3","authors_acknowledge":null,"authors_acknowledge_p":null},{"comment":"Typographical errors to correct: 'nuclesosynthesis' (§3), 'antrophic' (§4.1), 'whith' (§5), 'demostration' (Fig. 4 caption), and 'attained to' for 'attributed to' (§4.1 and Fig. 5 caption).","section":"Throughout","authors_acknowledge":null,"authors_acknowledge_p":null}],"recommendation":"major_revision"},"author_rebuttal":null,"desk_editor":{"model":"selfhosted/deepseek-v4.1-flash","letter":"This is Berezhiani's own review of the mirror-world cosmology program, and it reads best as a map rather than as a new result. The BBN bound x < 0.64 is standard and correctly applied, the GUT-baryogenesis comparison (k' = kx², D decreasing, so B' > B) is a fair parametric argument, and the qualitative picture — a colder sector freezes out earlier, so where the ordinary sector sits nearer equilibrium the mirror asymmetry is less damped — is coherent. The value is in the synthesis and in the exchange-leptogenesis section, which pulls together refs. 12–13. The paper is candid that it is a review, and the abstract's claims (s3, s4) are consistent with that framing.","headline":"A useful map of the mirror-world program, but the headline β ≈ 5 rests on a Boltzmann equation that does not match the equation it is solved from.","tokens_in":29856,"tokens_out":2501,"duration_ms":47001},"pith_extraction":{"msc":[],"pacs":["95.35.+d","98.80.Cq","12.60.-i","14.60.Pq"],"model":"selfhosted/deepseek-v4.1-flash","headline":"If a mirror copy of our particle physics were reheated colder than ours, its baryon asymmetry would survive better and its baryons could be the dark matter.","keywords":["mirror matter","mirror baryons","dark matter","baryogenesis","leptogenesis","kinetic mixing","big bang nucleosynthesis","mirror parity"],"falsifier":"Precision CMB anisotropy and galaxy power-spectrum data can settle the mirror-baryon dark matter case: if mirror baryons make up all of the dark matter, the paper's own spectra show a strong deficit of small-scale power for $x ≳ 0.3$, so a confirmed measurement of the matter spectrum at $k/h ∼ 0.2$ Mpc$^{-1}$ that matches cold dark matter while the BBN limit still permits $x$ near $0.5$ would exclude the scenario in that regime. A separate handle is a dedicated $e^+e^- →$ invisible search reaching $ε ∼ 10^{-9}$, which tests the kinetic-mixing portal that the scenario needs if mirror matter is to be detected at all.","tokens_in":30015,"feed_emoji":"🪞","tokens_out":4634,"duration_ms":79292,"temperature":0.7,"pith_summary":"The paper asks what happens to a universe that contains an exact mirror copy of our particle physics — the same gauge groups, couplings and masses — but which was reheated to a lower temperature than our sector. Nucleosynthesis limits force mirror photons, electrons and neutrinos to be cooler by a fixed ratio $x = T'/T < 0.64$; otherwise they would add too much radiation to the early expansion. Berezhiani argues that this one number, which stays essentially constant through cosmic expansion, makes every key epoch in the mirror world — baryogenesis, nucleosynthesis, photon decoupling — run under different conditions than in ours. The payoff is the claim that the mirror world ends up with a larger baryon asymmetry than the visible one, so that mirror baryons, invisible to our photons but otherwise ordinary matter, can supply the dark matter. If that is right, the near-coincidence of the visible and dark densities stops being a coincidence and becomes a consequence of two sectors sharing one microphysics at two temperatures.","feed_headline":"A colder mirror world should hold more baryons than ours","feed_subtitle":"If the mirror sector is cooler, its baryon asymmetry survives better — and mirror baryons can be the dark matter.","key_machinery":"The machinery is the depletion factor $D(k)$, the ratio of the realised baryon asymmetry to the asymmetry one would get if the relevant reactions were arbitrarily slow. It is defined by solving the Boltzmann equation for the asymmetry with a source term and an erasure term, giving $D(k) = (3/5)e^{-k}F(k) + (2/5)G(k)$ with $F$ and $G$ as in Eq. (47), normalised so that $D → 1$ as $k → 0$. Its role is to make the comparison between sectors quantitative: because the two sectors share microphysics, the same function $D$ applies to both, and the entire difference between them is carried by the rescaling $k → kx^2$ or $kx^3$. That single substitution is what turns a temperature ratio into a baryon-density ratio, and it is what makes the dark-to-visible ratio a calculable number rather than an input.","core_discovery":"The central claim is that a temperature difference between two otherwise identical sectors is enough to break the symmetry of their baryon contents in a definite direction: the colder sector gets more baryons. The mechanism is the standard out-of-equilibrium logic of baryogenesis, where the final asymmetry is suppressed by a damping factor $D(k)$ that depends on how long the relevant reactions stay in equilibrium, $k = (Γ/H)$ evaluated at the relevant epoch. In the mirror sector the Hubble rate is still dominated by the ordinary plasma, so the same reactions are slower relative to expansion, and the effective parameter is rescaled: $k' = kx^2$ for GUT-style decays and $k' = kx^3$ for the ordinary–mirror exchange leptogenesis of Section 4.3. Since $D$ decreases with $k$, the mirror asymmetry is always the less damped one, $B' > B$. The paper then converts this into a density ratio, $β = Ω'_b/Ω_b ≈ 1/D(k)$, and notes that $k ≈ 1.5$ gives $β ≈ 5$, which is the observed dark-to-visible ratio. Along the way it draws out the consequences of the same temperature gap for mirror nucleosynthesis (mirror helium $Y'_4 = 0.6$–$0.8$, against our $0.24$), for mirror recombination at $1+z'_{dec} ≈ 1100/x$, and for structure formation, where mirror Silk damping sets a smallest surviving perturbation mass of order $10^{11} M_⊙$ for $x$ near $0.3$ — a galaxy mass. The paper presents itself as a review, gathering earlier work on the GUT and electroweak cases and on exchange leptogenesis, and adding the cosmological survey of mirror baryon dark matter.","pith_inferences":["The two expressions the paper gives for the density ratio are not the same bookkeeping: the GUT-era formula carries an explicit entropy factor $x^3$ while the exchange-leptogenesis formula does not. If the $x^3$ version is the correct one, the $β ≈ 5$ fit moves to a different $k$, and since $k$ is tied to the same parameters that the CMB bounds on $x$ constrain, the two could in principle be check","Because mirror baryons are dissipative, mirror halos should cool and contract unless mirror star formation is fast enough to lock the gas into collisionless remnants. Comparing the inner density profiles of low-surface-brightness galaxies against the predicted mirror Silk mass would be a way to test the picture that does not require any non-gravitational coupling between the sectors.","The paper notes in a footnote that a temperature-dependent source term means hotter patches produce more $B-L$, generating isocurvature fluctuations correlated with the adiabatic ones. That is a distinctive and in principle measurable signature, and it is stated rather than computed; quantifying it against current CMB limits would be a natural next step.","A gravitational-wave background from a population of mirror supernovae is a channel that survives even if the sectors communicate by gravity alone, and it is the one prediction of the scenario that does not depend on the kinetic-mixing or neutrino-mixing portals being nonzero."],"forward_implications":["Mirror baryons as the whole of dark matter implies a cut-off in the matter power spectrum from mirror Silk damping, with the smallest surviving scale around $10^{11} M_⊙$ for $x ≈ 0.3$, comparable to a galaxy mass.","Mirror helium would be far more abundant than ordinary helium, $Y'_4 = 0.6$–$0.8$ versus $0.24$, so mirror stars would start from a different chemical composition and evolve on a different schedule.","Mirror recombination occurs at $1+z'_{dec} ≈ 1100/x$, earlier than ours; for $x < 0.3$ the mirror photons decouple while the universe is still radiation dominated.","Mirror stars above the Chandrasekhar limit would already have exploded, leaving roughly $0.5 M_⊙$ remnants as microlensing objects, which is the mass scale the microlensing data actually indicate.","Mirror supernovae would be dark in ordinary light but audible in gravitational waves, and in neutrinos if the ordinary and mirror neutrinos mix."],"supporting_citations":[{"why":"Supplies the comparison of ordinary and mirror baryogenesis in the GUT and electroweak cases, the mirror helium yield, and the mirror recombination, Jeans and Silk scale analysis that Section 5 builds on.","marker":"[11]"},{"why":"Origin of the ordinary–mirror exchange leptogenesis mechanism, the CP-asymmetry structure and the out-of-equilibrium treatment that Section 4.3 develops.","marker":"[12]"},{"why":"Gives the nucleosynthesis bound on photon kinetic mixing, $ε < 3 × 10^{-8}$, which caps how strongly the two sectors may communicate and hence supports the decoupling premise.","marker":"[4]"},{"why":"Provides the active–sterile neutrino mass matrix with mixed ordinary–mirror entries used for the neutrino portal and for the mirror-supernova neutrino signal.","marker":"[6]"},{"why":"Models in which the mirror sector is reheated to a lower temperature, and the bound $λ < 10^{-8}$ on the mixed Higgs quartic that keeps the sectors from re-equilibrating.","marker":"[9]"},{"why":"The WMAP values $Ω_b ≈ 0.044$ and $Ω_m ≈ 0.27$ that fix the target ratio $β ≈ 5$ the scenario is asked to reproduce.","marker":"[24]"},{"why":"Source of the depletion factor $D(k)$ obtained by solving the asymmetry Boltzmann equation beyond the $Γ ≪ H$ limit, quoted in Eq. (47).","marker":"[29]"},{"why":"The detailed CMB and large-scale-structure spectra behind the statement that $x ≳ 0.3$ is disfavoured when mirror baryons constitute all of the dark matter.","marker":"[31]"}],"fun_headline_variants":["Colder mirror sector should hold more baryons than ours","Mirror baryons can be the dominant dark matter","Temperature gap breaks baryon symmetry between sectors","Mirror helium should be 0.6 to 0.8, not 0.24","Mirror Silk damping sets smallest mass near a galaxy mass"],"cache_read_input_tokens":0,"weakest_assumption_plain":"The load-bearing premise is that the two sectors never return to thermal contact, so the mirror world stays colder throughout baryogenesis, and that the ratio of the two baryon densities is then given by the ratio of damping factors alone, $1/D(k)$, without the extra entropy factor $x^3$ that the paper's own GUT-era formula carries.","fun_headline_variants_meta":{"raw":{"variants":["Colder mirror sector should hold more baryons than ours","Mirror baryons can be the dominant dark matter","Temperature gap breaks baryon symmetry between sectors","Mirror helium should be 0.6 to 0.8, not 0.24","Mirror Silk damping sets smallest mass near a galaxy mass"]},"model":"selfhosted/deepseek-v4.1-flash","effort":"low","attempts":1,"cost_usd":0.0,"raw_usage":{"total_tokens":1765,"prompt_tokens":1028,"completion_tokens":737,"prompt_tokens_details":null,"completion_tokens_details":{"reasoning_tokens":664}},"tokens_in":1028,"tokens_out":737,"duration_ms":11976,"image_pages":[],"temperature":1.0,"reasoning_budget":50,"reasoning_tokens":664,"transport_provider":"selfhosted","cache_read_input_tokens":0,"cache_creation_input_tokens":0},"cache_creation_input_tokens":0},"created_at":"2026-11-13T08:55:59.975658+00:00","model_set":{"reader":"selfhosted/deepseek-v4.1-flash"},"pipeline_version":"pith-pipeline@v1.5.0-archive-selfhost","input_kind":null,"input_chars":null,"input_total_chars":null,"passes_missing":null,"published_standing":null,"published_confidence":null,"objection_audit":null,"run_record":null,"basis":{"kind":"not_recorded","source":null,"chars_given":null,"chars_total":null},"receipt":null,"falsifier":"Precision CMB anisotropy and galaxy power-spectrum data can settle the mirror-baryon dark matter case: if mirror baryons make up all of the dark matter, the paper's own spectra show a strong deficit of small-scale power for $x ≳ 0.3$, so a confirmed measurement of the matter spectrum at $k/h ∼ 0.2$ Mpc$^{-1}$ that matches cold dark matter while the BBN limit still permits $x$ near $0.5$ would exclude the scenario in that regime. A separate handle is a dedicated $e^+e^- →$ invisible search reaching $ε ∼ 10^{-9}$, which tests the kinetic-mixing portal that the scenario needs if mirror matter is to be detected at all.","supporting_citations":[{"cited_title":"Phys. Lett. B503, 362 (2001); A. Ignatiev and R.R. Volkas, Phys. Rev. D 68 , 023518","cited_arxiv_id":null,"evidence_quote":"Supplies the comparison of ordinary and mirror baryogenesis in the GUT and electroweak cases, the mirror helium yield, and the mirror recombination, Jeans and Silk scale analysis that Section 5 builds on."},{"cited_title":"Phys. Rev. Lett. 87, 231304","cited_arxiv_id":null,"evidence_quote":"Origin of the ordinary–mirror exchange leptogenesis mechanism, the CP-asymmetry structure and the out-of-equilibrium treatment that Section 4.3 develops."},{"cited_title":"Phys. Lett. B193, 168","cited_arxiv_id":null,"evidence_quote":"Gives the nucleosynthesis bound on photon kinetic mixing, $ε < 3 × 10^{-8}$, which caps how strongly the two sectors may communicate and hence supports the decoupling premise."},{"cited_title":"Z. Berezhiani and G. Senjanovi´ c, Phys. Rev. Lett. 69, 3013 (1992); Z. Berezhiani and R.N. Mohapatra, Phys. Rev. D 52 , 6607","cited_arxiv_id":null,"evidence_quote":"Provides the active–sterile neutrino mass matrix with mixed ordinary–mirror entries used for the neutrino portal and for the mirror-supernova neutrino signal."},{"cited_title":"Phys. Lett. B375, 26 (1996); Z. Berezhiani, Acta Phys. Pol. B 27 , 1503","cited_arxiv_id":null,"evidence_quote":"Models in which the mirror sector is reheated to a lower temperature, and the bound $λ < 10^{-8}$ on the mixed Higgs quartic that keeps the sectors from re-equilibrating."},{"cited_title":"Spergel et al., Astrophys","cited_arxiv_id":null,"evidence_quote":"The WMAP values $Ω_b ≈ 0.044$ and $Ω_m ≈ 0.27$ that fix the target ratio $β ≈ 5$ the scenario is asked to reproduce."},{"cited_title":null,"cited_arxiv_id":null,"evidence_quote":"Source of the depletion factor $D(k)$ obtained by solving the asymmetry Boltzmann equation beyond the $Γ ≪ H$ limit, quoted in Eq. (47)."},{"cited_title":"Structure Formation with Mirror Dark Matter: CMB and LSS","cited_arxiv_id":"astro-ph/0312605","evidence_quote":"The detailed CMB and large-scale-structure spectra behind the statement that $x ≳ 0.3$ is disfavoured when mirror baryons constitute all of the dark matter."}],"lane_accuracy":{"status":"not yet measured","lane":{"model":"selfhosted/deepseek-v4.1-flash","input_kind":null},"url":"https://pith.science/accuracy"},"review_version":1}