REVIEW
Leptogenesis from Gravity Waves in Models of Inflation
High Energy Physics - Theory · Submitted 5 Mar 2004 · 16 references
Pith's verdict: A genuinely new anomaly-plus-birefringence mechanism, honestly presented, but the realistic-size claim rests on pushing the cutoff to the edge of the effective theory's stated validity.
T0 · AI review
Why Pith says this
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Referee report
The paper
The paper claims
Lepton number can be generated by the gravitational anomaly sourced by elliptically polarized inflationary gravitational waves, but only reaches the observed baryon asymmetry when the cutoff and Hubble scale sit at the boundary of the effective theory.
The reading
Extended reading notes
Core claim
The paper claims that the gravitational anomaly in the lepton number current, sourced by elliptically polarized gravity waves generated during inflation when the inflaton has a CP-odd component, can produce the observed cosmic matter asymmetry. Its final result is Eq. 31: n/s around 6.3 times 10 to the minus 4 times (H/M_Pl) to the 3/2 times (mu/M_Pl) cubed. The authors state that to recover the observed n/s of 2.4 times 10 to the minus 10, one needs (mu/M_Pl) squared around 10 to the minus 5 times (M_Pl/H), with H at its current upper bound and mu around M_Pl.
Load-bearing premise
The load-bearing premise is that the ultraviolet cutoff mu can be taken to the Planck scale while the effective field theory, which the paper itself says is valid only for mu < F, remains trustworthy. The mu-to-the-fourth enhancement in Eq. 26 and the mu-cubed scaling in Eq. 31 are what make the asymmetry large enough; at mu around H around 2 times 10 to the 14 GeV the paper's own estimate gives n/s around 10 to the minus 22, which it calls unsatisfactory. The realistic-size claim therefore rests on extrapolating the anomalous source term to the boundary of its stated domain of validity.
Original abstract
We present a new mechanism for creating the observed cosmic matter-antimatter asymmetry which satisfies all three Sakharov conditions from one common thread, gravitational waves. We generate lepton number through the gravitational anomaly in the lepton number current. The source term comes from elliptically polarizated gravity waves that are produced during inflation if the inflaton field contains a CP-odd component. In simple inflationary scenarios, the generated matter asymmetry is very small. We describe some special conditions in which our mechanism can give a matter asymmetry of realistic size.
The compiled record
The paper's own sentences, arranged, kept beside the review and separate from it. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.
The abstract, sentence by sentence
We present a new mechanism for creating the observed cosmic matter-antimatter asymmetry which satisfies all three Sakharov conditions from one common thread, gravitational waves. We generate lepton number through the gravitational anomaly in the lepton number current. The source term comes from elliptically polarizated gravity waves that are produced during inflation if the inflaton field contains a CP-odd component. In simple inflationary scenarios, the generated matter asymmetry is very small. We describe some special conditions in which our mechanism can give a matter asymmetry of realistic size.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We present a new mechanism for creating the observed cosmic matter-antimatter asymmetry which satisfies all three Sakharov conditions from one common thread, gravitational waves. | contribution 1.00 | 0.90 | 0.77 | asserted 1.00 |
| s1 | We generate lepton number through the gravitational anomaly in the lepton number current. | method 0.76 | 0.82 | 0.12 | asserted 1.00 |
| s2 | The source term comes from elliptically polarizated gravity waves that are produced during inflation if the inflaton field contains a CP-odd component. | method 0.94 | 0.66 | 0.10 | asserted 0.82 |
| s3 | In simple inflationary scenarios, the generated matter asymmetry is very small. | limitation 0.83 | 0.81 | 0.07 | asserted 1.00 |
| s4 | We describe some special conditions in which our mechanism can give a matter asymmetry of realistic size. | contribution 0.67 | 0.86 | 0.19 | asserted 0.62 |
What was examined, and what was not
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References
How later papers used it
176 later papers cite it
1 later paper by other authors is listed below: 1 used its method or tool. 1 more paper by the same authors is listed: 1 built on it.
Builds on it 1 paper · 1 by the same authors
By the same authors
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Built on this paper to present a mechanism that paves a possible way to generate net-lepton asymmetry by realizing the Sakharov conditions during inflation through dynamically intra-converting gauge field fluctuations into lepton asymmetry.
Chern-Simons Inflation and Baryogenesis (2011) (same authors) · 0.81 · paraphrased: the licence does not allow quoting
Uses its method or tool 1 of 3 papers with this label
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Reviewed chiral gravitational wave generation in models with a gCS term following this paper and imposed constraints on the model parameters to avoid ghost instability.
Gravitational leptogenesis with kination and gravitational reheating (2019) · 0.86 · paraphrased: the licence does not allow quoting
How the literature uses it
128 arXiv papers cite this in 223 sentences
Papers whose main result relates to this one's
States a conflicting result 1 paper
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We show how the mechanism recently proposed by Alexander, Peskin, and Sheikh-Jabbari, in which the observed cosmic matter-antimatter asymmetry comes from the contribution of the cosmological tensor perturbations to the gravitational anomaly in the Standard Model, does not work.
Note about leptogenesis from gravity waves in models of inflation · 0.96
Papers citing it · 149 sentences without a confident label
Contests it 2 papers
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As we shall show in the following sections of the current article, this has effects on the final estimate of the gravitational CS anomaly condensate, which during the inflationary era, considered in [ref] , is found here to be half of the value evaluated in that work.
Condensate-Induced Inflation from Primordial Gravitational Waves in String-Inspired Chern-Simons Gravity · Gravitational Waves in Chern-Simons Gravity · contest 0.82
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While the basic mechanism of gravitational leptogenesis from chiral gravitational wave production during inflation is robust, the original model proposed in Ref. [ref] has a number of issues.
Gravitational Leptogenesis, Reheating, and Models of Neutrino Mass · Gravitational leptogenesis · contest 0.80
Builds on it 1 paper
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The mechanism that we pave a possible way to generate the net-lepton asymmetry by realizing the Sakharov conditions [ref] during inflation by dynamically intra-converting the gauge field fluctuations into the lepton asymmetry of the universe, building on previous work of [ref] .
Chern-Simons Inflation and Baryogenesis · Introduction · 0.81
Uses its method or tool 3 papers
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Let us first review the chiral gravitational wave generation in the models with a gCS term following Ref. [ref] and impose the constraints on the model parameters to avoid ghost instability as is done in Ref. [ref] .
Gravitational leptogenesis with kination and gravitational reheating · The consistency of the model with the gravitational Chern-Simons term during inflation · 0.86
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On substituting [ref] and [ref] in [ref], then, and performing the Fourier integrations, up to an UV cutoff $μ$ [ref] , such that $k ≤a(η) μ$, we obtain to first order in $Θ$: [ref] : [equation] Passing from a conformal to Robertson-Walker cosmic time, we write $Θ= 4 f̈ + 8 H ḟ$.
Lorentz Symmetry Violation in String-Inspired Effective Modified Gravity Theories · Chiral-gravitational-wave quantized perturbations · 0.81
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Assuming a GW perturbation with metric, say: $ds^2 = dt^2 - a^2(t) [(1 - h_+(t,z)) dx^2 + (1 + h_+(t,z)) dy^2 + 2h_×(t,z) dx dy + dz^2 ]$, with the scale factor of the Universe being given by $a(t) ∼e^H_I t,$ where $H_I$ is approximately constant, corresponding to the inflation scale, we evaluate the gravitational anomaly condensate, following [ref] , by integrating over graviton modes with momenta up to an UltraViolet (UV) cut-off scale $μ$: [equation] to leading order in the slow-roll parameter $Θ= √(2/3) α^' κ/12 H_I ḃ ≪ 1$, with the overdot denoting derivative with respect to the cosmic time $t$ in the Robertson-Walker frame.
Going beyond the Standard paradigm of Cosmology: Torsion, gravitational anomalies and inflation without inflaton fields · Running-Vacuum-Model Inflation without Inflaton fields · 0.95
Uses its data or values 1 paper
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For our purposes we adopt the estimates for the anomaly condensate [ref], which are based on the classical analysis of [ref] .]) [equation] to leading order in the slow-roll parameter [equation] with $H$ the (approximately) constant Hubble parameter during inflation.
Primordial Black Holes and Gravitational Waves in Multi-Axion-Chern-Simons Inflation · Gravitational-Anomaly Condensates and Running Vacuum Inflation · 0.91
Compares with it 3 papers
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Then $k$-integration in [ref] gives lepton number density [equation] This is essentially the same result as Alexander et al. [ref] .
Gauss-Bonnet Chern-Simons gravitational wave leptogenesis · Introduction · 1.00
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Such a result yields a contribution which is two times larger than that of the redefinition function [ref], leading to a two times larger result for the condensate [ref], which was the case of [ref] .
Condensate-Induced Inflation from Primordial Gravitational Waves in String-Inspired Chern-Simons Gravity · The constancy of $⟨R_CS⟩$ · 0.91
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Roughly speaking, this is the opposite process as discussed in gravi-leptogenesis [ref] .
Gauge Field and Fermion Production during Axion Inflation · Inflation · 0.83
Cites it as support 1 paper
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Such a coupling arises naturally in a variety of frameworks: (i) in heterotic string theories upon 4-dimensional compactification and a low-energy expansion [ref] ; (ii) in loop quantum gravity when the Barbero Immirzi parameter is promoted to a field and coupled to fermions [ref] ; (iii) in effective field theories of inflation [ref] ; (iv) in dynamical Chern-Simons gravity [ref] .
Gravitational-Wave Mediated Preheating · Action and Evolution Equations · 0.97
Cites it as background 52 papers
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The gravitational leptogenesis scenario [ref] is a novel mechanism to produce the lepton asymmetry from the chiral gravitational waves generated during inflation with a gCS coupling through the gravitational anomaly in the lepton current.
Gravitational leptogenesis with kination and gravitational reheating · Discussion · 0.98
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An alternative possibility is gravitational leptogenesis, which consists in exploiting the chiral gravitational anomaly [ref] present in the Standard Model (that is, in the presence of only left-handed neutrinos[Even if right-handed neutrinos are added to the Standard Model, this anomaly is still present once they are integrated out, at sufficiently low energies [ref] .]), [equation] where $RR̃=(1/2)ϵ^μν_ρσR_μναβR^ρσαβ$ denotes the contraction between the Riemann tensor and its dual, and the factor $N_L-R=3$ arises from the difference between the number of left- and right-handed neutrinos in the theory.[In general, all chiral fermions in the theory contribute to $N_L-R$, with the contribution of each particle weighted by its corresponding $B-L$ factor (see e.g. [ref] ), but since the Standard Model contains an equal amount of left- and right-handed quarks, their contribution vanishes and
Induced gravitational waves and baryon asymmetry fluctuations from primordial black hole formation · Introduction · 0.86
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The model of leptogenesis proposed by Alexander, Peskin and Sheikh-Jabbari [ref] uses elliptically polarized gravitational waves as the source of the lepton asymmetry.
Gauss-Bonnet Chern-Simons gravitational wave leptogenesis · Introduction · 0.84
Discussion
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