Papers & Preprints (Click on the title to show/hide the abstract) 
33 
Blowup dynamics for smooth finite energy radial data solutions to the selfdual ChernSimonsSchrödinger equation, with S. Kwon and K. Kim. arXiv:2010.03252 [math.AP]
Abstract: We consider the finitetime blowup dynamics of solutions to the selfdual ChernSimonsSchrödinger (CSS) equation (also referred to as the JackiwPi model) near the radial soliton $Q$ with the least $L^2$norm (ground state). While a formal application of pseudoconformal symmetry to $Q$ gives rise to an $L^2$continuous curve of initial data sets whose solutions blow up in finite time, they all have infinite energy due to the slow spatial decay of $Q$. In this paper, we exhibit initial data sets that are smooth finite energy radial perturbations of $Q$, whose solutions blow up in finite time. Interestingly, their blowup rate differs from the pseudoconformal rate by a power of logarithm. Applying pseudoconformal symmetry in reverse, this also yields a first example of an infinitetime blowup solution, whose blowup profile contracts at a logarithmic rate.
Our analysis builds upon the ideas of previous works of the first two authors on (CSS) [21,22], as well as the celebrated works on energycritical geometric equations by Merle, Raphaël, and Rodnianski [33,38]. A notable feature of this paper is a systematic use of nonlinear covariant conjugations by the covariant CauchyRiemann operators in all parts of the argument. This not only overcomes the nonlocality of the problem, which is the principal challenge for (CSS), but also simplifies the structure of nonlinearity arising in the proof.

32 
Asymptotic stability of harmonic maps on the hyperbolic plane Under the Schrödinger maps evolution, with A. Lawrie, J. Lührmann and S. Shahshahani, to appear in Comm. Pure Appl. Math. arXiv:1909.06899 [math.AP]
Abstract: We consider the Cauchy problem for the Schrödinger maps evolution when the domain is the hyperbolic plane. An interesting feature of this problem compared to the more widely studied case on the Euclidean plane is the existence of a rich new family of finite energy harmonic maps. These are stationary solutions, and thus play an important role in the dynamics of Schrödinger maps. The main result of this article is the asymptotic stability of (some of) such harmonic maps under the Schrödinger maps evolution. More precisely, we prove the nonlinear asymptotic stability of a finite energy equivariant harmonic map $Q$ under the Schrödinger maps evolution with respect to nonequivariant perturbations, provided $Q$ obeys a suitable linearized stability condition. This condition is known to hold for all equivariant harmonic maps with values in the hyperbolic plane and for a subset of those maps taking values in the sphere. One of the main technical ingredients in the paper is a globalintime local smoothing and Strichartz estimate for the operator obtained by linearization around a harmonic map, proved in the companion paper.

31 
On the Cauchy problem for the Hall and electron magnetohydrodynamic equations without resistivity I: illposedness near degenerate stationary solutions, with I.J. Jeong. arXiv:1902.02025 [math.AP]
Abstract: In this article, we prove various illposedness results for the Cauchy problem for the incompressible Hall and electronmagnetohydrodynamic (MHD) equations without resistivity. These PDEs are fluid descriptions of plasmas, where the effect of collisions is neglected (no resistivity), while the motion of the electrons relative to the ions (Hall current term) is taken into account. The Hall current term endows the magnetic field equation with a quasilinear dispersive character, which is key to our mechanism for illposedness.
Perhaps the most striking conclusion of this article is that the Cauchy problems for the HallMHD (either viscous or inviscid) and the electronMHD equations, under one translational symmetry, are illposed near the trivial solution in any sufficiently high regularity Sobolev space $H^{s}$. This result holds despite obvious wellposedness of the linearized equations near the trivial solution, as well as conservation of the nonlinear energy, by which the $L^{2}$ norm (energy) of the solution stays constant in time. The core illposedness (or instability) mechanism is degeneration of certain high frequency wave packet solutions to the linearization around a class of linearly degenerate stationary solutions of these equations, which are essentially dispersive equations with degenerate principal symbols.
The results in this article are complemented by a companion work, where we provide geometric conditions on the initial magnetic field that ensure wellposedness(!) of the Cauchy problems for the incompressible Hall and electronMHD equations. In particular, in stark contrast to the results here, it is shown in the companion work that the nonlinear Cauchy problems are wellposed near any nonzero constant magnetic field.

30  Local smoothing estimates for Schrödinger equations on hyperbolic space, with A. Lawrie, J. Lührmann and S. Shahshahani. arXiv:1808.04777 [math.AP]
Abstract: We establish globalintime frequency localized local smoothing estimates for Schrödinger equations on hyperbolic space $\mathbb{H}^{d}$. In the presence of symmetric first and zeroth order potentials, which are possibly timedependent, possibly large, and have sufficiently fast polynomial decay, these estimates are proved up to a localized lower order error. Then in the timeindependent case, we show that a spectral condition (namely, absence of threshold resonances) implies the full local smoothing estimates (without any error), after projecting to the continuous spectrum. In the process, as a means to localize in frequency, we develop a general LittlewoodPaley machinery on $\mathbb{H}^{d}$ based on the heat flow. Our results and techniques are motivated by applications to the problem of stability of solitary waves to nonlinear Schrödingertype equations on $\mathbb{H}^{d}$.
As a testament of the robustness of approach, which is based on the positive commutator method and a heat flow based LittlewoodPaley theory, we also show that the main results are stable under small timedependent perturbations, including polynomially decaying second order ones, and small lower order nonsymmetric perturbations.

(The following four papers constitute a series, whose overview is provided in the summary below.) 
29  The YangMills heat flow and the caloric gauge, with D. Tataru. arXiv:1709.08599 [math.AP].
Abstract: This is the first part of the fourpaper sequence, which establishes the Threshold Conjecture and the Soliton Bubbling vs.~Scattering Dichotomy for the energy critical hyperbolic YangMills equation in the (4 + 1)dimensional Minkowski spacetime.
The primary subject of this paper, however, is another PDE, namely the energy critical YangMills heat flow on the 4dimensional Euclidean space. Our first goal is to establish sharp criteria for global existence and asymptotic convergence to a flat connection for this system in $\dot{H}^{1}$, including the Dichotomy Theorem (i.e., either the above properties hold or a harmonic YangMills connection bubbles off) and the Threshold Theorem (i.e., if the initial energy is less than twice that of the ground state, then the above properties hold). Our second goal is to use the YangMills heat flow in order to define the caloric gauge, which will play a major role in the analysis of the hyperbolic YangMills equation in the subsequent papers.

28  The hyperbolic YangMills equation in the caloric gauge. Local wellposedness and control of energy dispersed solutions, with D. Tataru, Pure Appl. Anal. Vol. 2 (2020) no. 2, pp. 233384. arXiv:1709.09332 [math.AP].
Abstract: This is the second part in a fourpaper sequence, which establishes the Threshold Conjecture and the Soliton Bubbling vs. Scattering Dichotomy for the hyperbolic YangMills equation in the (4+1)dimensional spacetime. This paper provides the key gaugedependent analysis of the hyperbolic YangMills equation.
We consider topologically trivial solutions in the caloric gauge, which was defined in the first paper using the YangMills heat flow. In this gauge, we establish a strong form of local wellposedness, where the time of existence is bounded from below by the energy concentration scale. Moreover, we show that regularity and dispersive behavior of the solution persists as long as energy dispersion is small. We also observe that fixedtime regularity (but not dispersive) properties in the caloric gauge may be transferred to the temporal gauge without any loss, proving as a consequence small data global wellposedness in the temporal gauge.
The results in this paper are used in the subsequent papers to prove the sharp Threshold Theorem in caloric gauge in the trivial topological class, and the dichotomy theorem in arbitrary topological classes.

27  The hyperbolic YangMills equation for connections in an arbitrary topological class, with D. Tataru, Comm. Math. Phys. Vol. 365 (2019), no. 2, pp. 683739. arXiv:1709.08604 [math.AP].
Abstract: This is the third part of a fourpaper sequence, which establishes the Threshold Conjecture and the SolitonBubbling vs. Scattering Dichotomy for the energy critical hyperbolic YangMills equation in the (4+1)dimensional Minkowski spacetime. This paper provides basic tools for considering the dynamics of the hyperbolic YangMills equation in an arbitrary topological class at an optimal regularity. We generalize the standard notion of a topological class of connections on $\mathbb{R}^{d}$, defined via a pullback to the onepoint compactification $\mathbb{S}^{d} = \mathbb{R}^{d} \cup \{ \infty \}$, to rough connections with curvature in the critical space $L^{d/2}(\mathbb{R}^{d})$. Moreover, we provide excision and extension techniques for the YangMills constraint (or Gauss) equation, which allow us to efficiently localize YangMills initial data sets. Combined with the results in the previous papers in the sequence, we obtain local wellposedness of the hyperbolic YangMills equation on $\mathbb{R}^{1+d}$ (d≥4) in an arbitrary topological class at optimal regularity in the temporal gauge (where finite speed of propagation holds). In addition, in the energy subcritical case d=3, our techniques provide an alternative proof of the classical finite energy global wellposedness theorem of KlainermanMachedon, while also removing the smallness assumption in the temporalgauge local wellposedness theorem of Tao.
Although this paper is a part of a larger sequence, the materials presented in this paper may be of independent and general interest. For this reason, we have organized the paper so that it may be read separately from the sequence.

26  The threshold conjecture for the energy critical hyperbolic YangMills equation, with D. Tataru. arXiv:1709.08606 [math.AP].
Abstract: This article represents the fourth and final part of a fourpaper sequence whose aim is to prove the Threshold Conjecture as well as the more general Dichotomy Theorem for the energy critical 4+1 dimensional hyperbolic YangMills equation. The Threshold Theorem asserts that topologically trivial solutions with energy below twice the ground state energy are global and scatter. The Dichotomy Theorem applies to solutions in arbitrary topological class with large energy, and provides two exclusive alternatives: Either the solution is global and scatters, or it bubbles off a soliton in either finite time or infinite time.
Using the caloric gauge developed in the first paper, the continuation/scattering criteria established in the second paper, and the large data analysis in an arbitrary topological class at optimal regularity in the third paper, here we perform a blowup analysis which shows that the failure of global wellposedness and scattering implies either the existence of a soliton with at most the same energy bubbling off, or the existence existence of a nontrivial selfsimilar solution. The proof is completed by showing that the latter solutions do not exist.

(The following two papers constitute a series; for an overview, see Section 1.1 of Paper 25.) 
25  Strong cosmic censorship in spherical symmetry for twoended asymptotically flat initial data I. The interior of the black hole region, with J. Luk, Ann. of Math. Vol. 190 (2019), no. 1, pp. 1111. arXiv:1702.05715 [grqc].
Abstract: This is the first and main paper of a twopart series, in which we prove the $C^{2}$formulation of the strong cosmic censorship conjecture for the EinsteinMaxwell(real)scalarfield system in spherical symmetry for twoended asymptotically flat data. For this model, it is known through the works of Dafermos and DafermosRodnianski that the maximal globally hyperbolic future development of any admissible twoended asymptotically flat Cauchy initial data set possesses a nonempty Cauchy horizon, across which the spacetime is $C^{0}$futureextendible (in particular, the $C^{0}$formulation of the strong cosmic censorship conjecture is false). Nevertheless, the main conclusion of the present series of papers is that for a generic (in the sense of being open and dense relative to appropriate topologies) class of such data, the spacetime is futureinextendible with a Lorentzian metric of higher regularity (specifically, $C^{2}$).
In this paper, we prove that the solution is $C^{2}$futureinextendible under the condition that the scalar field obeys an $L^{2}$averaged polynomial lower bound along each of the event horizons. This, in particular, improves upon a previous result of Dafermos, which required instead a pointwise lower bound. Key to the proof are appropriate stability and instability results in the interior of the black hole region, whose proofs are in turn based on ideas from the work of DafermosLuk on the stability of Kerr Cauchy horizon (without symmetry) and from our previous paper on linear instability of ReissnerNordström Cauchy horizon. In the second paper of the series, which concerns analysis in the exterior of the black hole region, we show that the $L^{2}$averaged polynomial lower bound needed for the instability result indeed holds for a generic class of admissible twoended asymptotically flat Cauchy initial data.

24  Strong cosmic censorship in spherical symmetry for twoended asymptotically flat initial data II. The exterior of the black hole region, with J. Luk, Ann. PDE. Vol. 5 (2019) no. 1. arXiv:1702.05716 [grqc].
Abstract: This is the second and last paper of a twopart series in which we prove the $C^{2}$formulation of the strong cosmic censorship conjecture for the EinsteinMaxwell(real)scalarfield system in spherical symmetry for twoended asymptotically flat data. In the first paper, we showed that the maximal globally hyperbolic future development of an admissible asymptotically flat Cauchy initial data set is $C^{2}$futureinextendible provided that an $L^{2}$averaged (inverse) polynomial lower bound for the derivative of the scalar field holds along each horizon. In this paper, we show that this lower bound is indeed satisfied for solutions arising from a generic set of Cauchy initial data. Roughly speaking, the generic set is open with respect to a (weighted) $C^{1}$ topology and is dense with respect to a (weighted) $C^{\infty}$ topology. The proof of the theorem is based on extensions of the ideas in our previous work on the linear instability of ReissnerNordström Cauchy horizon, as well as a new large data asymptotic stability result which gives good decay estimates for the difference of the radiation fields for small perturbations of an arbitrary solution.

23  Dynamical black holes with prescribed masses in spherical symmetry, with J. Luk and S. Yang, Proceedings of the Seventh International Congress of Chinese Mathematicians, Adv. Lect. Math., Vol. II (2019), no. 44, pp. 367387. arXiv:1702.05717 [grqc].
Abstract: We review our recent work on a construction of spherically symmetric global solutions to the Einsteinscalar field system with large bounded variation norms and large Bondi masses. We show that similar ideas, together with Christodoulou's short pulse method, allow us to prove the following result: Given $M_{i} \geq M_{f} > 0$ and $\epsilon > 0$, there exists a spherically symmetric (black hole) solution to the Einsteinscalar field system such that up to an error of size $\epsilon$, the initial Bondi mass is $M_{i}$ and the final Bondi mass is $M_{f}$. Moreover, if one assumes a continuity property of the final Bondi mass (which in principle follows from known techniques in the literature), then for $M_{i}> $M_{f} >0$, the above result holds without an $\epsilon$error.

22  Solutions to the Einsteinscalarfield system in spherical symmetry with large bounded variation norms, with J. Luk and S. Yang, Ann. PDE. Vol. 4 (2018), no. 1, Art. 3. arXiv:1605.03893 [grqc].
Abstract: It is wellknown that small, regular, spherically symmetric characteristic initial data to the Einsteinscalarfield system which are decaying towards (future null) infinity give rise to solutions which are fowardintime global (in the sense of future causal geodesic completeness). We construct a class of spherically symmetric solutions which are global but the initial norms are consistent with initial data not decaying towards infinity. This gives the following consequences: (1) We prove that there exist fowardintime global solutions with arbitrarily large (and in fact infinite) initial bounded variation (BV) norms and initial Bondi masses. (2) While general solutions with nondecaying data do not approach Minkowski spacetime, we show using the results of LukOh that if a sufficiently strong asymptotic flatness condition is imposed on the initial data, then the solutions we construct (with large BV norms) approach Minkowski spacetime with a sharp inverse polynomial rate. (3) Our construction can be easily extended so that data are posed at past null infinity and we obtain solutions with large BV norms which are causally geodesically complete both to the past and to the future. Finally, we discuss applications of our method to construct global solutions for other nonlinear wave equations with infinite critical norms.

21  Global wellposedness of high dimensional MaxwellDirac for small critical data, with C. Gavrus, Mem. Amer. Math. Soc. Vol. 264 (2020), no. 1279. arXiv:1604.07900 [math.AP]
Abstract: In this paper, we prove global wellposedness of the massless MaxwellDirac equation in Coulomb gauge on $\mathbb{R}^{1+4}$ ($d \geq 4$) for data with small scalecritical Sobolev norm, as well as modified scattering of the solutions. Main components of our proof are A) uncovering null structure of MaxwellDirac in the Coulomb gauge, and B) proving solvability of the underlying covariant Dirac equation. A key step for achieving both is to exploit (and justify) a deep analogy between MaxwellDirac and MaxwellKleinGordon (for which an analogous result was proved earlier by KriegerSterbenzTataru), which says that the most difficult part of MaxwellDirac takes essentially the same form as MaxwellKleinGordon.

20  Small data global existence and decay for relativistic ChernSimons equations, with M. Chae, Annales Henri Poincaré Vol 18 (2017), no. 6, 21232198. arXiv:1512.03039 [math.AP]
Abstract: We establish a general small data global existence and decay theorem for ChernSimons theories with a general gauge group, coupled with a massive relativistic field of spin 0 or 1/2. Our result applies to a wide range of relativistic ChernSimons theories considered in the literature, including the abelian/nonabelian selfdual ChernSimonsHiggs equation and the ChernSimonsDirac equation. A key idea is to develop and employ a gauge invariant vector field method for relativistic ChernSimons theories, which allows us to avoid the long range effect of charge.

19  The Cauchy problem for wave maps on hyperbolic space in dimensions d≥4, with A. Lawrie and S. Shahshahani, Int. Math. Res. Not. (IMRN) 2018, no. 7, 19542051. arXiv:1510.04296 [math.AP]
Abstract: We establish global wellposedness and scattering for wave maps from ddimensional hyperbolic space into Riemannian manifolds of bounded geometry for initial data that is small in the critical Sobolev space for d≥4. The main theorem is proved using the moving frame approach introduced by Shatah and Struwe. However, rather than imposing the Coulomb gauge we formulate the wave maps problem in Tao's caloric gauge, which is constructed using the harmonic map heat flow. In this setting the caloric gauge has the remarkable property that the main `gauged' dynamic equations reduce to a system of nonlinear scalar wave equations on ℍd that are amenable to Strichartz estimates rather than tensorial wave equations (which arise in other gauges such as the Coulomb gauge) for which useful dispersive estimates are not known. This last point makes the heat flow approach crucial in the context of wave maps on curved domains.

(The following two papers are parts of the preprint arXiv:1402.2305, split per journal's request.) 
18  On Nonperiodic Euler Flows with Hölder Regularity, with P. Isett, Arch. Rational Mech. Anal. (ARMA) Vol. 221 (2016), No. 2, pp. 725804. preprint.
Abstract: In [Ise13], the first author proposed a strengthening of Onsager’s conjecture on the failure of energy conservation for incompressible Euler flows with Hölder regularity not exceeding 1/3. This stronger form of the conjecture implies that anomalous dissipation will fail for a generic Euler flow with regularity below the Onsager critical space $L^{\infty}_{t} B^{1/3}_{3, \infty}$ due to low regularity of the energy profile.
This paper is the first and the main paper in a series of two papers, whose results may be viewed as first steps towards establishing the conjectured failure of energy regularity for generic solutions with Hölder exponent less than 1/5. The main result of the present paper shows that any given smooth Euler flow can be perturbed in $C^{1/5  \epsilon}_{t,x}$ on any precompact subset of $\mathbb{R} \times \mathbb{R}^{1+3}$ to violate energy conservation. Furthermore, the perturbed solution is no smoother than $C^{1/5  \epsilon}_{t,x}$. As a corollary of this theorem, we show the existence of nonzero $C^{1/5  \epsilon}_{t,x}$ solutions to Euler with compact spacetime support, generalizing previous work of the first author [Ise12] to the nonperiodic setting.

17  On the Kinetic Energy profile of Hölder continuous Euler flows, with P. Isett, Annales d'IHP (C) Vol. 34 (2017), no. 3, pp. 711730. preprint.
Abstract: In [Ise13], the first author proposed a strengthening of Onsager’s conjecture on the failure of energy conservation for incompressible Euler flows with Hölder regularity not exceeding 1/3. This stronger form of the conjecture implies that anomalous dissipation will fail for a generic Euler flow with regularity below the Onsager critical space $L^{\infty}_{t} B^{1/3}_{3, \infty}$ due to low regularity of the energy profile.
The present paper is the second in a series of two papers whose results may be viewed as first steps towards establishing the conjectured failure of energy regularity for generic solutions with Hölder exponent less than 1/5. The main result of this paper shows that any nonnegative function with compact support and Hölder regularity 1/2 can be prescribed as the energy profile of an Euler flow in the class $C^{1/5  \epsilon}_{t,x}$. The exponent 1/2 is sharp in view of a regularity result of Isett [Ise13]. The proof employs an improved greedy algorithm scheme that builds upon that in Buckmaster–De Lellis–Székelyhidi [BDLS13].

16  Equivariant Wave Maps on the Hyperbolic Plane with Large Energy, with A. Lawrie and S. Shahshahani, Math. Res. Lett. Vol. 24 (2017), no. 4, 10851147. arXiv:1505.03728 [math.AP]
Abstract: In this paper we continue the analysis of equivariant wave maps from 2dimensional hyperbolic space into surfaces of revolution that was initiated in earlier papers. When the target is the hyperbolic plane we proved in an earlier work the existence and asymptotic stability of a 1parameter family of finite energy harmonic maps indexed by how far each map wraps around the target. Here we conjecture that each of these harmonic maps is globally asymptotically stable, meaning that the evolution of any arbitrarily large finite energy perturbation of a harmonic map asymptotically resolves into the harmonic map itself plus free radiation. Since such initial data exhaust the energy space, this is the soliton resolution conjecture for this equation. The main result is a verification of this conjecture for a nonperturbative subset of the harmonic maps

(The following three papers constitute a series; for an overview, see Sections 23 of Paper 13.) 
15  Local wellposedness of the (4+1)dimensional MaxwellKleinGordon equation, with D. Tataru, Ann. PDE. Vol. 2 (2016), No. 1. arXiv:1503.01560 [math.AP]
Abstract: This paper is the first part of a trilogy dedicated to a proof of global wellposedness and scattering of the (4+1)dimensional massless MaxwellKleinGordon equation (MKG) for any finite energy initial data. The main result of the present paper is a large energy local wellposedness theorem for MKG in the global Coulomb gauge, where the lifespan is bounded from below by the energy concentration scale of the data. Hence the proof of global wellposedness is reduced to establishing nonconcentration of energy. To deal with nonlocal features of MKG we develop initial data excision and gluing techniques at critical regularity, which might be of independent interest.

14  Energy dispersed large energy solutions to the (4+1) dimensional MaxwellKleinGordon equation, with D. Tataru, Amer. J. Math. Vol. 140 (2018), no. 1, pp. 182. arXiv:1503.01561 [math.AP]
Abstract: This article is devoted to the massless energy critical MaxwellKleinGordon system in 4+1 dimensions. In earlier work of the second author, joint with Krieger and Sterbenz, we have proved that this problem has global wellposedness and scattering in the Coulomb gauge for small initial data. This article is the second of a sequence of three papers of the authors, whose goal is to show that the same result holds for data with arbitrarily large energy. Our aim here is to show that large data solutions persist for as long as one has small energy dispersion; hence failure of global wellposedness must be accompanied with a nontrivial energy dispersion.

13  Finite energy global wellposedness and scattering of the (4+1) dimensional MaxwellKleinGordon equation, with D. Tataru, Invent. Math. Vol. 205, (2016), no. 3, pp. 781–877. arXiv:1503.01562 [math.AP]
Abstract: This article constitutes the final and main part of a threepaper sequence, whose goal is to prove global wellposedness and scattering of the energy critical MaxwellKleinGordon equation (MKG) on $\mathbb{R}^{1+4}$ for arbitrary finite energy initial data. Using the successively stronger continuation/scattering criteria established in the previous two papers, we carry out a blowup analysis and deduce that the failure of global wellposedness and scattering implies the existence of a nontrivial stationary or selfsimilar solution to MKG. Then, by establishing that such solutions do not exist, we complete the proof.

12  A refined threshold theorem for (1+2)dimensional wave maps into surfaces, with A. Lawrie, Comm. Math. Phys. Vol. 342, (2016), no. 3, pp. 989999. arXiv:1502.03435 [math.AP]
Abstract: The recently established threshold theorem for energy critical wave maps states that wave maps with energy less than that of the ground state (i.e., a minimal energy nontrivial harmonic map) are globally regular and scatter on (1+2)dimensional Minkowski space. In this note we give a refinement of this theorem when the target is a closed orientable surface by taking into account an additional invariant of the problem, namely the topological degree. We show that the sharp energy threshold for global regularity and scattering is in fact twice the energy of the ground state for wave maps with degree zero, whereas wave maps with nonzero degree necessarily have at least the energy of the ground state. We also give a discussion on the formulation of a refined threshold conjecture for the energy critical SU(2) YangMills equation on (1+4)dimensional Minkowski space.

11  Gap Eigenvalues and Asymptotic Dynamics of Geometric Wave Equations on Hyperbolic Space, with A. Lawrie and S. Shahshahani, J. Funct. Anal. Vol. 271 (2016), no. 11, pp. 31113161. arXiv:1502.00697 [math.AP]
Abstract: In this paper we study kequivariant wave maps from the hyperbolic plane into the 2sphere as well as the energy critical equivariant SU(2) YangMills problem on 4dimensional hyperbolic space. The latter problem bears many similarities to a 2equivariant wave map into a surface of revolution. As in the case of 1equivariant wave maps considered in an earlier paper, both problems admit a family of stationary solutions indexed by a parameter that determines how far the image of the map wraps around the target manifold. Here we show that if the image of a stationary solution is contained in a geodesically convex subset of the target, then it is asymptotically stable in the energy space. However, for a stationary solution that covers a large enough portion of the target, we prove that the Schrödinger operator obtained by linearizing about such a harmonic map admits a simple positive eigenvalue in the spectral gap. As there is no a priori nonlinear obstruction to asymptotic stability, this gives evidence for the existence of metastable states (i.e., solutions with anomalously slow decay rates) in these simple geometric models.

10  Proof of linear instability of the ReissnerNordström Cauchy horizon under scalar perturbations, with J. Luk, Duke Math. J. Vol. 166 (2017), no. 3, pp. 437493. arXiv:1501.04598 [grqc]
Abstract: It has long been suggested that solutions to linear scalar wave equation
$$ \Box_{g} \phi = 0 $$
on a fixed subextremal ReissnerNordström spacetime with nonvanishing charge are generically singular at the Cauchy horizon. We prove that generic smooth and compactly supported initial data on a Cauchy hypersurface indeed give rise to solutions with infinite nondegenerate energy near the Cauchy horizon in the interior of the black hole. In particular, the solution generically does not belong to $W^{1,2}_{loc}$. This instability is related to the celebrated blue shift effect in the interior of the black hole. The problem is motivated by the strong cosmic censorship conjecture and it is expected that for the full nonlinear EinsteinMaxwell system, this instability leads to a singular Cauchy horizon for generic small perturbations of ReissnerNordström spacetime. Moreover, in addition to the instability result, we also show as a consequence of the proof that Price's law decay is generically sharp along the event horizon.

9  Profile decomposition for wave equations on hyperbolic space with applications, with A. Lawrie and S. Shahshahani, Math. Ann. Vol. 365 (2016), no. 12, pp. 707803. arXiv:1410.5847 [math.AP]
Abstract: The goal for this paper is twofold. Our first main objective is to develop BahouriGerard type profile decompositions for waves on hyperbolic space. Recently, such profile decompositions have proved to be a versatile tool in the study of the asymptotic dynamics of solutions to nonlinear wave equations with large energy. With an eye towards further applications, we develop this theory in a fairly general framework, which includes the case of waves on hyperbolic space perturbed by a timeindependent potential. Our second objective is to use the profile decomposition to address a specific nonlinear problem, namely the question of global wellposedness and scattering for the defocusing, energy critical, semilinear wave equation on threedimensional hyperbolic space, possibly perturbed by a repulsive timeindependent potential. Using the concentration compactness/rigidity method introduced by Kenig and Merle, we prove that all finite energy initial data lead to a global evolution that scatters to linear waves in infinite time. This proof will serve as a blueprint for the arguments in a forthcoming work, where we study the asymptotic behavior of large energy equivariant wave maps on the hyperbolic plane.

8  Stability of stationary equivariant wave maps from the hyperbolic plane, with A. Lawrie and S. Shahshahani, Amer. J. Math. Vo. 139 (2017), no. 4, pp. 10851147. arXiv:1402.5981 [math.AP]
Abstract: In this paper we initiate the study of equivariant wave maps from 2d hyperbolic space into rotationally symmetric surfaces. This problem exhibits markedly different phenomena than its Euclidean counterpart due to the exponential volume growth of concentric geodesic spheres on the domain.
In particular, when the target is the 2sphere, we find a family of equivariant harmonic maps indexed by a parameter that measures how far the image of each harmonic map wraps around the sphere. These maps have energies taking all values between zero and the energy of the unique corotational Euclidean harmonic map, Q, from the Euclidean plane to the 2sphere, given by stereographic projection. We prove that the harmonic maps are asymptotically stable for values of the parameter smaller than a threshold that is large enough to allow for maps that wrap more than halfway around the sphere. Indeed, we prove Strichartz estimates for the operator obtained by linearizing around such a harmonic map. However, for harmonic maps with energies approaching the Euclidean energy of Q, asymptotic stability via a perturbative argument based on Strichartz estimates is precluded by the existence of gap eigenvalues in the spectrum of the linearized operator.
When the target is 2d hyperbolic space, we find a continuous family of asymptotically stable equivariant harmonic maps with arbitrarily small and arbitrarily large energies. This stands in sharp contrast to the corresponding problem on Euclidean space, where all finite energy solutions scatter to zero as time tends to infinity.

7  Quantitative decay rates for dispersive solutions to the Einsteinscalar field system in spherical symmetry, with J. Luk, Analysis & PDE. Vol. 8 (2015), No. 7, pp. 1603–1674. arXiv:1402.2984 [grqc]
Abstract: In this paper, we study the future causally geodesically complete solutions of the spherically symmetric Einsteinscalar field system. Under the a priori assumption that the scalar field $\phi$ scatters locally in the scaleinvariant boundedvariation (BV) norm, we prove that $\phi$ and its derivatives decay polynomially. Moreover, we show that the decay rates are sharp. In particular, we obtain sharp quantitative decay for the class of global solutions with small BV norms constructed by Christodoulou. As a consequence of our results, for every future causally geodesically complete solution with sufficiently regular initial data, we show the dichotomy that either the sharp power law tail holds or that the spacetime blows up at infinity in the sense that some scale invariant spacetime norms blow up.

6  Decay and scattering for the ChernSimonsSchrödinger equations, with F. Pusateri, Int. Math. Res. Not.. IMRN 2015 (2015), No. 24, pp. 1312213147 arXiv:1311.2088 [math.AP]
Abstract: We consider the ChernSimonsSchrödinger model in 1+2 dimensions, and prove scattering for small solutions of the Cauchy problem in the Coulomb gauge. This model is a gauge covariant Schrödinger equation, with a potential decaying like $r^{−1}$ at infinity. To overcome the difficulties due to this long range decay we start by performing $L^{2}$based estimates covariantly. This gives favorable commutation identities so that only curvature terms, which decay faster than $r^{−1}$, appear in our weighted energy estimates. We then select the Coulomb gauge to reveal a genuinely cubic null structure, which allows us to show sharp decay by Fourier methods.

5  A heat flow approach to Onsager's conjecture for the Euler equations on manifolds, with P. Isett, Trans. Amer. Math. Soc. Vol. 368 (2016), No. 9, pp. 65196537. arXiv:1310.7947 [math.AP]
Abstract: We give a simple proof of Onsager's conjecture concerning energy conservation for weak solutions to the Euler equations on any compact Riemannian manifold, extending the results of ConstantinETiti and CheskidovConstantinFriedlanderShvydkoy in the flat case. When restricted to $\mathbb{T}^{d}$ or $\mathbb{R}^{d}$, our approach yields an alternative proof of the sharp result of the latter authors.
Our method builds on a systematic use of a smoothing operator defined via a geometric heat flow, which was considered by MilgramRosenbloom as a means to establish the Hodge theorem. In particular, we present a simple and geometric way to prove the key nonlinear commutator estimate, whose proof previously relied on a delicate use of convolutions.

4  Finite energy global wellposedness of the ChernSimonsHiggs equations in the Coulomb gauge. arXiv:1310.3955 [math.AP]
Abstract: In a recent paper, SelbergTesfahun proved that the abelian ChernSimonsHiggs system (CSH) is globally wellposed for finite energy initial data under the Lorenz gauge condition. It has been suspected by Huh, however, that such a result should hold in the Coulomb gauge as well. In this note, we give an affirmative answer to this question by first establishing low regularity local wellposededness of (CSH) in the Coulomb gauge for initial data set $(f, g) \in H^{\gamma}_{x} \times H^{\gamma1}_{x}$ for any $\gamma > 3/4$. Then by conservation of energy, global wellposedness for (CSH) in the energy space $(f,g) \in H^{1}_{x} \times L^{2}_{x}$ follows rather immediately.

(The following two papers constitute a series; for an overview, see Section 1 of Paper 2.) 
3  Gauge choice for the YangMills equations using the YangMills heat flow and local wellposedness in H^{1}, J. Hyper. Diff. Equ. Vol. 11 (2014), No. 01, pp. 1 108. arXiv:1210.1558 [math.AP].
Abstract: n this work, we introduce a novel approach to the problem of gauge choice for the YangMills equation on the Minkowski space $\mathbb{R}^{1+3}$, which uses the YangMills heat flow in a crucial way. As this approach does not possess the drawbacks of the previous approaches, it is expected to be more robust and easily adaptable to other settings.
As the first demonstration of the `structure' offered by this new approach, we will give an alternative proof of the local wellposedness of the YangMills equations for initial data in $(\dot{H}^{1} \cap L^{3}_{x}) \times L^{2}_{x}$, which is a classical result of S. Klainerman and M. Machedon that had been proved using a different method (local Coulomb gauges). The new proof does not involve localization in spacetime, which had been the key drawback of the previous method. Based on the results proved in this paper, a new proof of finite energy global wellposedness of the YangMills equations, also using the YangMills heat flow, is established in a companion article.

2  Finite Energy Global Wellposedness of the YangMills equations on $\mathbb{R}^{1+3}$: An Approach Using the YangMills Heat Flow, Duke Math. J. Vol. 164 (2015), No. 9, pp. 16691732 arXiv:1210.1557 [math.AP].
Abstract: In this work, along with the companion work Oh (2012), we propose a novel approach to the problem of gauge choice for the YangMills equations on the Minkowski space $\mathbb{R}^{1+3}$. A crucial ingredient is the associated YangMills heat flow. As this approach does not possess the drawbacks of the previous approaches (as in KlainermanMachedon (1995) and Tao (2003)), it is expected to be more robust and easily adaptable to other settings.
Building on the results proved in the companion article Oh (2012), we prove, as one of the first applications of our approach, finite energy global wellposedness of the YangMills equations on $\mathbb{R}^{1+3}$. This is a classical result first proved by S. Klainerman and M. Machedon (1995) using local Coulomb gauges. As opposed to their method, the present approach avoids the use of Uhlenbeck's lemma (1982), and hence does not involve localization in spacetime.

1  Low regularity solutions to the ChernSimonsDirac and the ChernSimonsHiggs equations in the Lorenz gauge, with H. Huh, Comm. Partial Differential Equations. Vol. 41 (2016), no. 3, 989–999. arXiv:1209.3841[math.AP]
Abstract: In this paper, we address the problem of local wellposedness of the ChernSimonsDirac (CSD) and the ChernSimonsHiggs (CSH) equations in the Lorenz gauge for low regularity initial data. One of our main contributions is the uncovering of a null structure of (CSD). Combined with the standard machinery of $X^{s,b}$ spaces, we obtain local wellposedness of (CSD) for initial data $a_{\mu},\psi \in H^{1/4 + \epsilon}_{x}$. Moreover, it is observed that the same techniques applied to (CSH) lead to a quick proof of local wellposedness for initial data $a_{\mu} \in H^{1/4 + \epsilon}_{x}$, $(\phi, \partial_{t} \phi) \in H^{3/4 + \epsilon}_{x} \times H^{1/4+\epsilon}_{x}$, which improves the previous result of SelbergTesfahun (2012).
