The Newtonian Limit in CDT
  Adam Getchell (UC Davis) acgetchell@ucdavis.edu




Sunday, April 14, 13
Does CDT have a Newtonian Limit?

                       • CDT looks like GR at cosmological scales,
                         does it have a Newtonian limit?
                                       Gm1 m2
                                   F =
                                         r2
                       • At first glance, this is hard:
                         • CDT is not well suited for approximating
                           smooth classical space-times
                         • We don’t have the time or resolution to
                           watch objects fall

Sunday, April 14, 13
A trick from GR
                 •     The static axisymmetric Weyl metric

                                       ds2 = e2 dt2             e2(⌫    )
                                                                            dr2 + dz 2                         r2 e   2
                                                                                                                           d     2


                 •     With two-body solutions
                                                                                q
                                                           µ1      µ2                        2
                                              (r, z) =                , Ri = r2 + (z zi )
                                                           R1      R2
                                                                                 2
                                                µ2 r 2
                                                 1         µ2 r 2
                                                            2          4µ1 µ2    r + (z z1 ) (z                           z2 )
                                  ⌫(r, z) =        4          4   +           2                                                      1
                                                 R1         R2      (z1 z2 )           R1 R2

                 •     Leads to a “strut”
                                                                                4µ1 µ2
                                                                ⌫(0, z) =                      2
                                                                            (z1         z2 )

                 •     With a stress
                                                                  1 ⇣               ⌫(r,z)
                                                                                             ⌘
                                                         Tzz   =      1         e                  2⇡ (r)
                                                                 8⇡G


                 •     That can be integrated to get the Newtonian force
                                        Z
                                                      1 ⇣              ⌫(r,z)
                                                                                ⌘        Gm1 m2
                                  F =       Tzz dA =      1        e                =                      2    for   µi = Gmi
                                                     4G                                 (z1         z2 )



Sunday, April 14, 13
Measuring Mass in CDT

                       Mass ➔ Epp quasilocal energy
                                                    Z              p         ⇣p               p             ⌘
                                               1                                                  ¯    ¯2
                                       EE ⌘                 d2 x       | |        k2    l2        k2   l
                                              8⇡G       ⌦


                                                             µ⌫                    µ⌫
                                                l⌘                lµ⌫        k⌘         kµ⌫



                 •     In 2+1 CDT, extrinsic curvature at an edge is proportional to the number
                       of connected tetrahedra

                 •     In 3+1 CDT, extrinsic curvature at a face is proportional to the number of
                       connected pentachorons (4-simplices)




Sunday, April 14, 13
Measuring Mass in CDT

                       Mass ➔ Epp quasilocal energy
                                                    Z              p         ⇣p               p             ⌘
                                               1                                                  ¯    ¯2
                                       EE ⌘                 d2 x       | |        k2    l2        k2   l
                                              8⇡G       ⌦


                                                             µ⌫                    µ⌫
                                                l⌘                lµ⌫        k⌘         kµ⌫



                 •     In 2+1 CDT, extrinsic curvature at an edge is proportional to the number
                       of connected tetrahedra

                 •     In 3+1 CDT, extrinsic curvature at a face is proportional to the number of
                       connected pentachorons (4-simplices)




Sunday, April 14, 13
Some Computational Methods
                       • Distance
                         • Calculate single-source shortest path
                           between the two masses using Bellman-
                           Ford algorithm
                         • Modify allowed moves in a sweep to not
                           permit successive moves which increase or
                           decrease distance
                       • Stress
                           • Hmmm ...

Sunday, April 14, 13
On-Going work
                       • Based on Rajesh Kommu’s CDT implementation
                         • arxiv.org/abs/1110.6875
                       • Code is on GitHub (warning: messy!)
                         • https://github.com/ucdavis/CDT
                       • Work in early stages, results “soon”
                       • Thanks to Markus Afshar, Professor Steve
                         Carlip, Joshua Cooperman, Colin Cunliff,
                         Henrique Gomez, Rajesh Kommu, Jonah Miller,
                         and Charles Pierce for many helpful discussions

Sunday, April 14, 13

Newtonian limit in cdt

  • 1.
    The Newtonian Limitin CDT Adam Getchell (UC Davis) acgetchell@ucdavis.edu Sunday, April 14, 13
  • 2.
    Does CDT havea Newtonian Limit? • CDT looks like GR at cosmological scales, does it have a Newtonian limit? Gm1 m2 F = r2 • At first glance, this is hard: • CDT is not well suited for approximating smooth classical space-times • We don’t have the time or resolution to watch objects fall Sunday, April 14, 13
  • 3.
    A trick fromGR • The static axisymmetric Weyl metric ds2 = e2 dt2 e2(⌫ ) dr2 + dz 2 r2 e 2 d 2 • With two-body solutions q µ1 µ2 2 (r, z) = , Ri = r2 + (z zi ) R1 R2  2 µ2 r 2 1 µ2 r 2 2 4µ1 µ2 r + (z z1 ) (z z2 ) ⌫(r, z) = 4 4 + 2 1 R1 R2 (z1 z2 ) R1 R2 • Leads to a “strut” 4µ1 µ2 ⌫(0, z) = 2 (z1 z2 ) • With a stress 1 ⇣ ⌫(r,z) ⌘ Tzz = 1 e 2⇡ (r) 8⇡G • That can be integrated to get the Newtonian force Z 1 ⇣ ⌫(r,z) ⌘ Gm1 m2 F = Tzz dA = 1 e = 2 for µi = Gmi 4G (z1 z2 ) Sunday, April 14, 13
  • 4.
    Measuring Mass inCDT Mass ➔ Epp quasilocal energy Z p ⇣p p ⌘ 1 ¯ ¯2 EE ⌘ d2 x | | k2 l2 k2 l 8⇡G ⌦ µ⌫ µ⌫ l⌘ lµ⌫ k⌘ kµ⌫ • In 2+1 CDT, extrinsic curvature at an edge is proportional to the number of connected tetrahedra • In 3+1 CDT, extrinsic curvature at a face is proportional to the number of connected pentachorons (4-simplices) Sunday, April 14, 13
  • 5.
    Measuring Mass inCDT Mass ➔ Epp quasilocal energy Z p ⇣p p ⌘ 1 ¯ ¯2 EE ⌘ d2 x | | k2 l2 k2 l 8⇡G ⌦ µ⌫ µ⌫ l⌘ lµ⌫ k⌘ kµ⌫ • In 2+1 CDT, extrinsic curvature at an edge is proportional to the number of connected tetrahedra • In 3+1 CDT, extrinsic curvature at a face is proportional to the number of connected pentachorons (4-simplices) Sunday, April 14, 13
  • 6.
    Some Computational Methods • Distance • Calculate single-source shortest path between the two masses using Bellman- Ford algorithm • Modify allowed moves in a sweep to not permit successive moves which increase or decrease distance • Stress • Hmmm ... Sunday, April 14, 13
  • 7.
    On-Going work • Based on Rajesh Kommu’s CDT implementation • arxiv.org/abs/1110.6875 • Code is on GitHub (warning: messy!) • https://github.com/ucdavis/CDT • Work in early stages, results “soon” • Thanks to Markus Afshar, Professor Steve Carlip, Joshua Cooperman, Colin Cunliff, Henrique Gomez, Rajesh Kommu, Jonah Miller, and Charles Pierce for many helpful discussions Sunday, April 14, 13