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Modified Ricci Solitons in Geometry

Updated 14 July 2026
  • Modified Ricci solitons are Einstein-type metrics on complete Riemannian manifolds that incorporate an extra tensor term, generalizing Ricci solitons, n-quasi-Einstein metrics, and almost solitons.
  • They arise naturally from warped product constructions and conformal reductions, providing deep insights into flow dynamics and rigidity phenomena through modified Ricci-harmonic flows.
  • The theory offers explicit models, eigenvalue bounds, and rigidity results, while extending the framework to include flux-coupled and higher-order curvature modifications.

Modified Ricci solitons are a class of Einstein type metrics defined on a complete Riemannian manifold (Mm,g)(M^m,g) endowed with a vector field XX and a $1$-form ω\omega by

Ric+12LXg=λg+θωω,\operatorname{Ric}+\frac12\mathcal{L}_X g=\lambda g+\theta\,\omega\otimes\omega,

for real λ\lambda and θ>0\theta>0. In the gradient case, X=ηX=\nabla\eta and ω=dξ\omega=d\xi, so the equation becomes

Ric+dη=λg+θdξdξ.\operatorname{Ric}+\nabla d\eta=\lambda g+\theta\,d\xi\otimes d\xi.

This framework contains Ricci solitons and XX0-quasi-Einstein metrics, is closely related to warped product constructions, and arises as the self-similar sector of a modified Ricci-harmonic flow (Filho, 29 Sep 2025).

1. Defining equation and basic variants

The defining modified Ricci soliton equation is

XX1

Its gradient form is

XX2

If XX3 is allowed to be a nonconstant function, the structure is called a modified Ricci almost soliton (Filho, 29 Sep 2025).

The same source places modified Ricci solitons in direct relation with two established classes. Ricci solitons are recovered by setting XX4 and XX5, so that

XX6

The XX7-quasi-Einstein equation is

XX8

and is presented there as a special case of the modified Ricci soliton equation. In parallel, the theory of Ricci almost solitons replaces the constant soliton parameter in the classical gradient Ricci soliton equation by a smooth function: XX9 That construction generalizes gradient Ricci solitons and introduces the shrinking, steady, expanding, and indefinite cases according to the sign behavior of $1$0 (Pigola et al., 2010).

Structure Equation Relation stated in the literature
Modified Ricci soliton $1$1 General class
Gradient modified Ricci soliton $1$2 Gradient case
Ricci soliton $1$3 Obtained when $1$4, $1$5
$1$6-quasi-Einstein metric $1$7 Presented as a special case
Ricci almost soliton $1$8 Variable soliton function

A recurrent point of terminology is that “modified,” “almost,” and “generalized” do not denote the same alteration. The data indicate that modified Ricci solitons add a tensor term $1$9, whereas almost solitons replace the constant coefficient by a function. This suggests terminological caution when comparing results across subliteratures.

2. Warped products, quasi-Einstein metrics, and conformal reductions

A principal structural motivation for modified Ricci solitons is their relation to warped products. For a Ricci soliton realized as a warped product ω\omega0, the metric on the base ω\omega1 satisfies

ω\omega2

Letting ω\omega3, one has

ω\omega4

and therefore

ω\omega5

In this way, the base metric of a warped product Ricci soliton becomes a modified Ricci soliton with ω\omega6 and ω\omega7 (Filho, 29 Sep 2025).

The same warped-product viewpoint interacts with the quasi-soliton formalism. If ω\omega8 is a warped product gradient Ricci soliton, then the base metric ω\omega9 satisfies

Ric+12LXg=λg+θωω,\operatorname{Ric}+\frac12\mathcal{L}_X g=\lambda g+\theta\,\omega\otimes\omega,0

with Ric+12LXg=λg+θωω,\operatorname{Ric}+\frac12\mathcal{L}_X g=\lambda g+\theta\,\omega\otimes\omega,1. Under the functional dependence assumption Ric+12LXg=λg+θωω,\operatorname{Ric}+\frac12\mathcal{L}_X g=\lambda g+\theta\,\omega\otimes\omega,2, such a base metric is called a special quasi-soliton. For Kähler special quasi-solitons of real dimension at least four, the metric satisfies a Ricci-Hessian equation on an open set, and if that equation is standard then the metric is a Riemannian product; when Ric+12LXg=λg+θωω,\operatorname{Ric}+\frac12\mathcal{L}_X g=\lambda g+\theta\,\omega\otimes\omega,3, one factor is a Kähler-Einstein manifold of codimension Ric+12LXg=λg+θωω,\operatorname{Ric}+\frac12\mathcal{L}_X g=\lambda g+\theta\,\omega\otimes\omega,4 (Maschler, 2015).

Conformal reductions furnish an analogous route. If Ric+12LXg=λg+θωω,\operatorname{Ric}+\frac12\mathcal{L}_X g=\lambda g+\theta\,\omega\otimes\omega,5 is a gradient Ricci soliton conformal to a Kähler metric Ric+12LXg=λg+θωω,\operatorname{Ric}+\frac12\mathcal{L}_X g=\lambda g+\theta\,\omega\otimes\omega,6, then, in terms of Ric+12LXg=λg+θωω,\operatorname{Ric}+\frac12\mathcal{L}_X g=\lambda g+\theta\,\omega\otimes\omega,7,

Ric+12LXg=λg+θωω,\operatorname{Ric}+\frac12\mathcal{L}_X g=\lambda g+\theta\,\omega\otimes\omega,8

with the key hypothesis Ric+12LXg=λg+θωω,\operatorname{Ric}+\frac12\mathcal{L}_X g=\lambda g+\theta\,\omega\otimes\omega,9. In dimension λ\lambda0, the partial classification obtained under this hypothesis yields four possibilities on an open dense set: λ\lambda1 is a Kähler-Ricci soliton; λ\lambda2 satisfies a Ricci-Hessian equation; λ\lambda3 and λ\lambda4 is Einstein; or λ\lambda5 and λ\lambda6 is a non-Einstein steady gradient Ricci soliton (Maschler, 2015).

These constructions show that modified Ricci solitons are not merely formal perturbations of the Ricci soliton equation. They encode the effective geometry seen on the base of a warped product and, in the conformal-Kähler setting, reduce naturally to Ricci-Hessian type equations.

3. Flow interpretation and explicit models

Modified Ricci solitons appear as special solutions of the modified Ricci-harmonic flow

λ\lambda7

where λ\lambda8 is a family of maps and λ\lambda9 for a fixed θ>0\theta>00-form θ>0\theta>01 on θ>0\theta>02. A modified Ricci-harmonic soliton is a triple θ>0\theta>03 satisfying

θ>0\theta>04

and the self-similar solutions evolve by

θ>0\theta>05

This gives a direct dynamical interpretation of the modified Ricci soliton equation (Filho, 29 Sep 2025).

An explicit example is given by

θ>0\theta>06

with θ>0\theta>07 endowed with the Euclidean metric. Choosing

θ>0\theta>08

one verifies

θ>0\theta>09

Hence X=ηX=\nabla\eta0 realizes a modified Ricci-harmonic soliton and, after suitable scaling and diffeomorphism, a special solution to the modified Ricci-harmonic flow (Filho, 29 Sep 2025).

A related coupled theory is the harmonic-Ricci soliton system,

X=ηX=\nabla\eta1

with gradient version

X=ηX=\nabla\eta2

In that setting, the modified curvature quantities are the X=ηX=\nabla\eta3-Ricci tensor X=ηX=\nabla\eta4, the X=ηX=\nabla\eta5-scalar curvature X=ηX=\nabla\eta6, and the associated X=ηX=\nabla\eta7-Schouten, X=ηX=\nabla\eta8-Cotton, X=ηX=\nabla\eta9-Weyl, and ω=dξ\omega=d\xi0-Bach tensors (Anselli, 2020).

4. Rigidity, eigenvalue bounds, and dynamical stability

The compact theory includes a rigidity theorem in the spirit of Lichnerowicz and Obata. If ω=dξ\omega=d\xi1, ω=dξ\omega=d\xi2, is a compact modified Ricci almost soliton with constant scalar curvature ω=dξ\omega=d\xi3, and if ω=dξ\omega=d\xi4 is an eigenfunction of the Laplacian with eigenvalue ω=dξ\omega=d\xi5,

ω=dξ\omega=d\xi6

then

ω=dξ\omega=d\xi7

Equality holds if and only if ω=dξ\omega=d\xi8 is isometric to the standard sphere ω=dξ\omega=d\xi9, where

Ric+dη=λg+θdξdξ.\operatorname{Ric}+\nabla d\eta=\lambda g+\theta\,d\xi\otimes d\xi.0

and the structure is gradient, up to rescaling and addition of a constant (Filho, 29 Sep 2025).

The broader almost-soliton literature provides analogous rigidity and isolation phenomena. For Ricci almost solitons,

Ric+dη=λg+θdξdξ.\operatorname{Ric}+\nabla d\eta=\lambda g+\theta\,d\xi\otimes d\xi.1

the weighted Laplacian

Ric+dη=λg+θdξdξ.\operatorname{Ric}+\nabla d\eta=\lambda g+\theta\,d\xi\otimes d\xi.2

and the Bakry-Émery Ricci tensor

Ric+dη=λg+θdξdξ.\operatorname{Ric}+\nabla d\eta=\lambda g+\theta\,d\xi\otimes d\xi.3

play a central role. The theory derives differential identities such as

Ric+dη=λg+θdξdξ.\operatorname{Ric}+\nabla d\eta=\lambda g+\theta\,d\xi\otimes d\xi.4

together with existence, rigidity, a-priori curvature estimates, isolation phenomena, and topological consequences under weighted maximum principles and volume comparison (Pigola et al., 2010).

Dynamical stability is developed for a curvature-normalized Ricci flow

Ric+dη=λg+θdξdξ.\operatorname{Ric}+\nabla d\eta=\lambda g+\theta\,d\xi\otimes d\xi.5

whose stationary solutions satisfy

Ric+dη=λg+θdξdξ.\operatorname{Ric}+\nabla d\eta=\lambda g+\theta\,d\xi\otimes d\xi.6

Using weighted little Hölder spaces, maximal regularity theory, and Simonett’s theorem, strict linear stability implies dynamical stability for a class of Einstein metrics and for a class of non-Einstein Ricci solitons, with many explicit examples on simply connected solvable Lie groups (Williams et al., 2013). In this sense, rigidity and stability enter the modified-soliton landscape both through elliptic characterizations and through normalized flow dynamics.

5. Flux-coupled and higher-order modifications

One major extension of the Ricci soliton paradigm introduces a closed Ric+dη=λg+θdξdξ.\operatorname{Ric}+\nabla d\eta=\lambda g+\theta\,d\xi\otimes d\xi.7-form Ric+dη=λg+θdξdξ.\operatorname{Ric}+\nabla d\eta=\lambda g+\theta\,d\xi\otimes d\xi.8. Generalized Ricci solitons are pairs Ric+dη=λg+θdξdξ.\operatorname{Ric}+\nabla d\eta=\lambda g+\theta\,d\xi\otimes d\xi.9 satisfying

XX00

The steady, gradient, XX01-invariant case on XX02 reduces to the ansatz

XX03

and yields the ODE system

XX04

For each XX05 below the threshold XX06, the resulting local solution extends to a complete, positively curved, XX07-invariant, steady generalized Ricci soliton of gradient type, and varying XX08 gives a one-parameter family of pairwise non-isometric metrics (Podestà et al., 2024).

The Heterotic-Ricci flow introduces both a XX09-form XX10 and a non-negative parameter XX11: XX12 When XX13, it reduces to the generalized Ricci flow; when XX14 and XX15, it reduces to a constrained version of the RG-2 flow. The corresponding Heterotic soliton equations involve XX16, XX17, the curvature square term XX18, and the Bianchi identity. In dimension three, compact strong Heterotic solitons are classified, up to finite cover, as hyperbolic three-manifolds or quotients of the Heisenberg group equipped with a left-invariant metric; moreover, all Einstein three-dimensional Heterotic solitons have constant dilaton, and Einstein Heterotic solitons with constant dilaton are rigid (Moroianu et al., 2023).

These theories extend the modified-soliton idea beyond an added XX19 term. They incorporate torsion, flux, and higher-curvature corrections while preserving the central soliton principle: stationary or self-similar behavior for a geometric flow after allowing diffeomorphisms and, in some settings, scaling.

6. Special geometries, Lorentzian models, and curvature-modified classifications

On Sasaki-like almost contact B-metric manifolds, a Ricci-like soliton with arbitrary potential vector field XX20 is defined by

XX21

For a Sasaki-like manifold of dimension XX22, any such soliton with constants XX23 must satisfy

XX24

and its Ricci tensor is

XX25

The scalar curvatures relative to XX26 and XX27 are both constant and equal to XX28. In the gradient almost Ricci-like case,

XX29

the soliton coefficients are proved to be constant, and explicit XX30- and XX31-dimensional Lie group examples are exhibited (Manev, 2020).

A Lorentzian counterpart appears in the study of conformal Ricci-Bourguignon solitons on Vaidya spacetime. There the soliton equation is

XX32

and the Vaidya metric in Eddington-Finkelstein coordinates is

XX33

With XX34 and XX35, the admissible vector field coefficients reduce to

XX36

where XX37. In the gradient case, when XX38,

XX39

The decisive rigidity result is that the PDE system is compatible only when the mass function vanishes, XX40, so such solitons exist only in flat Minkowski spacetime; no genuinely radiating Vaidya spacetime admits them (Rehman et al., 13 Aug 2025).

A different curvature modification appears in four-dimensional gradient shrinking Ricci solitons through the modified curvature tensor

XX41

and the associated modified sectional curvature XX42. In dimension four, if

XX43

then the soliton is locally Kähler. For compact solitons with lower bounds on XX44 and XX45, the gap theorems stated in the source force the manifold to be isometric to XX46 or XX47, and a Hitchin-Thorpe type inequality is obtained under positive modified sectional curvature (Cao et al., 25 Sep 2025).

Across these examples, the common theme is that a “modified” Ricci soliton equation typically acquires extra tensorial data—XX48-forms, fluxes, torsion, conformal terms, auxiliary metrics, or curvature corrections—and that the resulting flexibility is often sharply constrained by rigidity, classification, or stability theorems.

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