background the linear schr odinger equation iu t u does
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Background: The linear Schr odinger equation iu t = u does not - PowerPoint PPT Presentation

A Limiting Absorption Principle for Dirac Operators in Two and Higher Dimensions Michael Goldberg , University of Cincinnati joint work with Burak Erdogan , University of Illinois and William Green , Rose-Hulman AMS Northeastern Sectional Meeting


  1. A Limiting Absorption Principle for Dirac Operators in Two and Higher Dimensions Michael Goldberg , University of Cincinnati joint work with Burak Erdogan , University of Illinois and William Green , Rose-Hulman AMS Northeastern Sectional Meeting Buffalo, NY September 17, 2017 Support provided by Simons Foundation grant #281057.

  2. Background: The linear Schr¨ odinger equation iu t = − ∆ u does not respect special relativity. Relationships between velocity, momentum, and energy follow Newtonian mechanics. − u tt = ( − ∆ + m 2 ) u The Klein-Gordon equation has the right relationship between these quantities, but it doesn’t have a unitary evolution. �� − ∆ + m 2 � The equation iu t = u is unitary and encodes special relativity, but the operator is nonlocal. This makes it unclear how to add electromagnetic fields.

  3. The Dirac System in R n : Let α 1 , . . . , α n and β be anti-commuting matrices with α 2 j = I = β 2 . When n = 2 it is convenient to use the Pauli spin matrices. n � � � Define the Dirac operator D m := − i α j ∂ j + mβ . j =1 Thanks to the anti-commutation properties, D 2 m = − ∆ + m 2 . Then the free Dirac equation is i u t = D m u

  4. Not too surprisingly, solutions of the free Dirac equation satisfy the same Strichartz inequalities as the Klein-Gordon equation, � � � �∇� − θ e − itD m u � � x � � u � L 2 � L p t L q with the admissibility conditions 2 p + n q = n θ ≥ 1 2 + 1 p − 1 2 , when m > 0 . q [D’Ancona-Fanelli, Cacciafesta] Or if m = 0, then the wave equation Strichartz estimates apply: � � � |∇| − θ e − itD m u � � x � � u � L 2 � L p t L q with the admissibility conditions 2 p + n − 1 = n − 1 2 − 1 θ = n p − n , q . q 2

  5. We’d like to know if a perturbed Dirac operator D m + V ( x ) yields the same bounds. Here V is a Hermitian matrix with each ( � x � − 1 − ǫ if m = 0). entry bounded pointwise by � x � − 2 − ǫ Spectral properties: The essential spectrum of D m is ( −∞ , − m ] ∪ [ m, ∞ ). The spectrum of D m + V has no singular continuous part, or embedded eigenvalues or resonances [Georgescu-Mantoiu]. Threshold resonances and eigenvalues are possible, along with a finite point spectrum inside ( − m, m ).

  6. Theorem (Erdogan-G-Green) : If V ( x ) is continuous and has the specified pointwise decay, and there are no threshold resonances or eigenvalues, then the semigroup e − i ( D m + V ) t P ac u satisfies the same Strichartz bounds as the corresponding free Dirac equation.

  7. Short proof: First establish uniform bounds on the resolvent ( D m + V − ( λ ± iε )) − 1 for all | λ | ∈ [ m, ∞ ). � � | V | 1 / 2 ( D m + V − ( λ ± iε )) − 1 | V | 1 / 2 � � � In particular, show that � 2 → 2 has a uniform bound. Kato smoothing arguments lead to a weighted bound in L 2 t,x for both the free and perturbed Dirac evolution. Then an argument due to Rodnianski-Schlag parlays these into Strichartz estimates for the perturbed equation. Remark: Only the first part is new, and it turns out most of the work has been done before.

  8. In fact, Georgescu-Mantoiu already proved uniform resolvent bounds on any compact interval inside of | λ | ∈ ( m, λ 1 ]. That leaves one big task. Theorem (E-G-G) : If V ( x ) has continuous entries bounded by � x � − 1 − ǫ , then there exist constants λ 1 < ∞ and δ > 0 so that the operator norm � � | V | 1 / 2 ( D m + V − ( λ ± iε )) − 1 | V | 1 / 2 � � � � 2 → 2 is bounded uniformly over | λ | > λ 1 and 0 < ǫ < δ | λ | . It is not necessary for V ( x ) to be Hermitian for this result. And a smaller task to do the same in a neighborhood of λ = ± m .

  9. The uniform bound for ( D m − λ ) − 1 is well known. The perturbation identity I + V ( D m − λ ) − 1 � − 1 ( D m + V − λ ) − 1 = ( D m − λ ) − 1 � would be immediately useful if the operator norm of ( D m − λ ) − 1 decayed as λ → ∞ . It doesn’t. Using the fact that D 2 m = − ∆ + m 2 , we can rewrite the last factor as � − 1 � − 1 . � � − ∆ − ( λ 2 − m 2 ) I + V ( D m + λ ) � �� � � �� � 1 st -order Schr¨ odinger resolvent This has a lot in common with magnetic Schr¨ odinger operators! (with magnetic potential V · ∇ )

  10. Uniform resolvent bounds for magnetic Schr¨ odinger operators: Positive commutator methods [Robert, D’Ancona-Fanelli-Cacciafesta]. Straightforward integration by parts. Needs some differentiabilty of V ( x ). Also need n − 3 ≥ 0. Directional decomposition of the resolvent [E-G-G]. Constructs the operator inverse via convergent power series. Complicated estimates of iterated integrals. May sometimes need differentiability of V ( x ) when n = 2 (but not this time).

  11. Remarks about the λ = m threshold: If m > 0, this regime is identical a Schr¨ odinger operator near λ = 0. Resolvent expansions [Jensen, Kato, Nenciu] are known. The m = 0 case is quite different. For example, the resolvent of ( − ∆) in R 2 has a resonance at λ = 0. The resolvent of a massless Dirac operator D 0 doesn’t. For future study: • Low-energy resolvent expansions when m = 0. • Classification of threshold obstructions. • Pointwise dispersive estimates. • L p -boundedness of the wave operators?

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