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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

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Newtonian limit in cdt

  • 1. The Newtonian Limit in CDT Adam Getchell (UC Davis) acgetchell@ucdavis.edu Sunday, April 14, 13
  • 2. 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
  • 3. 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
  • 4. 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
  • 5. 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
  • 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