3D Dirac operator

3D Dirac operator

The three dimensional space \mathbb{R}^3 is important because we live in it. With the scalar Laplacian -\Delta in dimension q=3, the Hydrogen operator -\Delta + 1/r (leaving out constants) essentially explains the periodic system of elements and so the starting point of chemistry. The eigenvalue difference 1/n^2 - 1/m^2 explain spectral lines (like Lyman (UV light) , Balmer (visible light) , Paschen (infrared light) ). The integral operator expressions for the inverse of the Laplacian explain why the electromagnetic or gravitational potentials have the form 1/r. The three dimensional integral calculus is taught in multi-variable calculus courses, where the exterior derivative grad, curl and div appear. One usually does not write down the Dirac operator on all differential forms. There are 0 forms, 1 forms, 2 forms and 3 forms. We usually identify 0 and 3 forms and 1 and 2 forms. The curl of a vector field is still considered to be a vector field. The Dirac operator in flat 3 dimensional space is D = \left[ \begin{array}{cccc} 0 & -{\rm grad}^* & 0 & 0 \\ {\rm grad} & 0 & {\rm -curl}^* & 0 \\ 0 & {\rm curl} & 0 & {\rm -div}^* \\ 0 & 0 & {\rm div} & 0 \end{array} \right]. The Hodge Laplacian L=D^2 has 4 diagonal blocks containing the scalar Laplacian L_0 = -\Delta. For 3-forms, it looks the same just L_3 f dxdydz = -\Delta f dxdydz. On 1-forms and 2-forms which in multi-variable calculus always are identified as “vector fields”, one would write there L_1 ( P dx + Q dy + R dz) = -\Delta P dx  -\Delta Q dy - \Delta R dz and similarly for 2-forms P dydz + Q dxdz + R dxdy. The solution of the wave equation in 3 dimensional space u_{tt} = \Delta u can be written down conveniently as u(t) = \cos(Dt) u(0) + t {\rm sinc}(Dt) u'(0). And now we can note that \cos = \phi_1 and {\rm sinc}= \phi_3 are Bessel functions. This triggered me to talk on Saturday about a PDE riddle. The path u(t) = \phi_k u(0) is a solution of a modified wave equation u_{tt} = - D^2 u - (k-1) u_t/t as the computation in the box below shows. I had hoped that u(t) = \phi_k u(0) + t \phi_{k+2} u'(0) would more generally solve this wave equation; but this did not pan out: for the velocity part, it only fits for k=1, where it is the usual wave equation and where \phi_{3} ={\rm sinc} is the sinc function.

A PDE attempt:

Motivated by the fact that u(t) \phi_1(tD)  u(0) + t \phi_3(tD)  u''(0) solves the wave equation u_{tt} + D^2 u=0 on an arbitrary Riemannian q-manifold, we attempted to see whether in general, u(t) = \phi_k(tD) u(0) + \phi_{k+2}(tD) u'(0) satisfies a modified PDE. Here, $\phi_q(r)$ solves the Bessel differential equation \phi''(r) + (q-1) phi'(r) /r + phi(r) =0 with the initial condition \phi(0)=1, \phi'(0)=0. The first cases are \phi_1(r) = \cos(r), \phi_2(r) = J_0(r) , \phi_3(r) = {\rm sinc}(r) = \sin(r)/r, \phi_4(r) = 2 J_1(r)/r and \phi_5(r) =  \frac{\sin (r)-r \cos (r)}{r^3}. Since the d’Alembert type formula u(t) = \phi_1(tD) u(0) + t \phi_3(tD) u'(0) satisfies the wave equation u_{tt} = - D^2 u on a general Riemannian manifold (M,g) with Dirac operator D=d+d^*, the square root of the Hodge Laplacian d d^* + d^* d, it was tempting to explore whether \phi_k(tD) + \phi_{k+2}(tD) satisfies this PDE. On Saturday morning, I thought it does, but if done correctly, there is an annoying single term \phi_{q+2} u'(0)  (q-1)/t left, when trying with the wave type equation u_{tt} + D^2 u + u_t (q-1)/t = 0. (The computation is below). The reason, why I would have liked it is because it would give more intuition about why D_t f = \phi_{q+2}(tD) Df is a good deformation of the Dirac operator. What we know is that D_t f(p) is completely determined by f only on W_t(p) the wave front. In dimension q, we need $\latex \phi_{q+2}$ when doing sphere averages and I still wonder why q+2 and not q in dimension q. It is clear in 1-dimension, where \phi_3= {\rm sinc} is needed to get the discrete derivative [f(x+t)-f(x-t)] /2.

Upshot: the form u(t) = \phi_q(tD) f satisfies the PDE u_{tt}+D^2 u + (q-1) u_t/t=0 with u(0)=f. The path u(t)=t \phi_{q+2}(tD) f does not satisfy this PDE with initial velocity $u_t(0)=f$ however. The question had been triggered by the fact that the expression d_t f = \phi_{q+2} (tD) df is a nice deformed exterior derivative that uses the wave front at distance t.

Just to recall, the starting point had been that d_t f = \phi_{q+2} (tD) df is the flux of f through W_t(p) if f is a $(q-1)$-form. This was a consequence of the Jeffrey Ovall formulas for sphere or ball averages. One can deduce from this that the Huygens property holds for all differential forms and not only q-1 forms. Using the magical Cartan formula for the Lie derivative L_X = i_X d + d i_X, one can in generalsee by taking inner derivatives that also for general k-forms, the formula d_t f produces an exterior derivative that only uses f on the wave front: one just has to write every differential form as a linear combination of decomposable forms i_X g, where g is invariant under the flow of X like i_{e^1}  g(y) dx= g(y) or i_{e^2} g(x) dy = g(x) or i_{e^1+e^2} g(x-y) (d(x+y)) = g(x-y) in the case q=2 and derive the Huygens principle for k=0 forms if it is known for k=1 forms. Why do we see the Bessel case q+2 in the sphere averages in dimension q? The PDE u_{tt} + D^2 u + u_t (q-1)/t almost works for the velocity. It does for position, but for velocity there is a term left. If the initial velocity u_t(0)=0 is zero, then u(t) = \phi_q(tD) u(0) satisfies this modified wave PDE. It would have been nice (and was wishful thinking triggered by the 1- dimensional case) to explain better the q+2 Bessel solution appearing in the exterior derivative d_t f = \phi_{q+2}(tD) df that is the center of attention as it has the property that d_t f(p) only depends on the wave front W_t(p). There is a cancellation explaining a bit the shift from the q-Bessel equation f''+(q-1) f/r + f=0 to the (q+2)-Bessel equation f''+(q+1) f/r = f=0 solved by \phi_{q+2}, but it is not enough.

Attempt: is it true that u = f_q u(0)  + t f_{q+2} u'(0)  = f X + t g Y
solves the PDE           u_tt + D^2 u + u_t (q-1)/t   where f_q  solves
the Bessel equation f''(r) + (q-1) f'(r)/r  + f(r) = 0,  f(0)=1, f'(0)=0         ?

Write u(0) = X and  u'(0) = Y   for the initial position and initial velocity.
Write simply f = f(tD) =f_q(tD)  and     g = g(tD) = f_{q+2}(tD) and use

Bessel  f''(tD) + (q-1) f'(tD)/(tD) + f(tD) = 0                (*)
Bessel  g''(tD) + (q+1) g'(tD)/(tD) + g(tD) = 0                (**)
chain rule :   d/dt f(tD) = f'(tD) D  and   d^2/dt^2  f(tD) =    f''(tD) D^2  

       POSITION                          MOMENTUM
------------------------------------------------------------------------------
u    = f       X                   + t g     Y    
u_t  = f'  D   X                   + t g'  D Y               +   g    Y     
u_tt = f'' D^2 X                   + t g'' D^2 Y  +  g' D Y  +   g' D Y
------------------------------------------------------------------------------            

Multiply the first equation by D^2, the second by (q-1)/t and switch q-1 to q+1
with      t g' D^2 Y (q-1)/(tD)  =   t g' D^2 Y (q+1)/(tD)    - 2 g' D Y    

------------------------------------------------------------------------------            
D^2 u       = f   D^2 X            + t g   D^2 Y    
u_t (q-1)/t = f'  D^2 X (q-1)/(tD) + t g'  D^2 Y (q+1)/(tD) + g Y (q-1)/t - 2g' D Y
u_tt        = f'' D^2 X            + t g'' D^2 Y            + 2g' D Y  
------------------------------------------------------------------------------

              Bessel  (q-1)          Bessel (q+1)   
 Adds to 0    Add to 0               Add to zero              g Y (q-1)/t    
 by PDE       by (*)                 by (**)                  Remains