Search
Search Funnelback University
- Refined by:
- Date: 2015
31 -
40 of
1,134
search results for KaKaoTalk:ZA31 24 24
where 0
match all words and 1,134
match some words.
Results that match 2 of 3 words
-
Cylindrically Symmetric Systems in GaugeTheory Gravity Jeffrey…
geometry.mrao.cam.ac.uk/wp-content/uploads/2015/02/97Cylindrical_Systems_Thesis.pdf16 Feb 2015: h(a) 7 h′(a) = Rh(a)R̃ (1.24). andω(a) 7 ω′(a) = Rω(R̃aR)R̃ 2LR̃aRRR̃, (1.25). ... Using (2.24) and the above constraints, the Einstein equations take thereduced form. -
comp_paper.dvi
geometry.mrao.cam.ac.uk/wp-content/uploads/2015/02/97tunnelling_times.pdf16 Feb 2015: This involves a configuration spacewith multiple time coordinates, and may be regarded as the relativistic generalisationof the multiparticle Bohmian approach [24]. ... Phys. Rev.A, 51:2748, 1995. [24] P.R. Holland. The Quantum Theory of Motion. -
arXiv:astro-ph/9804150v1 16 Apr 1998
geometry.mrao.cam.ac.uk/wp-content/uploads/2015/02/9804150_CovariantCMB.pdf18 Feb 2015: S2Q(k) [12] satisfying. Q̇(k) = O(1). Specifically, we have. X (i)a =. k. kX (i)k Q(k)a , Za =. k. k2. SZkQ(k)a (2.24). -
arXiv:gr-qc/0405033v1 6 May 2004
geometry.mrao.cam.ac.uk/wp-content/uploads/2015/02/98_Gravity_Gauge.pdf18 Feb 2015: Anumber of other helpful introductory articles can be found, including those byHestenes [35, 36], Vold [24, 28], and Doran & Lasenby [37]. ... 3.24). Hence µRR̃ is equal to minus its reverse and so must be a bivector. -
kschild1.dvi
geometry.mrao.cam.ac.uk/wp-content/uploads/2015/02/98kerr_schild1.pdf18 Feb 2015: Ricci Tensor: R(b) aR(ab) (24)Ricci Scalar: R aR(a) (25). Einstein Tensor: G(a) R(a) 12aR. -
kschild2.dvi
geometry.mrao.cam.ac.uk/wp-content/uploads/2015/02/98kerr_schild2.pdf18 Feb 2015: For the formerwe note that. (αn)2α. =α2 β2. 2α=. (α′n)2α′. (24). ... 24. -3. -2. -1. 0. 1. 2. 3. 0 1 2 3 4 5. -
torsion.dvi
geometry.mrao.cam.ac.uk/wp-content/uploads/2015/02/98spin_torsion.pdf18 Feb 2015: Hanson. Gravitation, gauge theories anddifferential geometry. Phys. Rep., 66(6):213, 1980. 24. ... Class. Quantum.Grav., 2:919, 1985. [24] A. Barducci, R. Casalbuoni, and L. -
arXiv:astro-ph/9810123v1 8 Oct 1998
geometry.mrao.cam.ac.uk/wp-content/uploads/2015/02/99AnisotropiesI.pdf19 Feb 2015: H(t) =Ṡ(t). S(t), (24). so that. Γ2 = 1 kr2/S2, (25). ... 0.24. 0.26. 0 0.2 0.4 0.6 0.8 1 1.2. r (arbitrary units). -
Geometric algebra and the causal approachto multiparticle quantum…
geometry.mrao.cam.ac.uk/wp-content/uploads/2015/02/99Causal.pdf19 Feb 2015: Employing the one-particleidentity. ik1B1ik. 1B1, 5.24. we see that with no sum over a. -
Classical and Quantum Dynamics in a Black Hole Background
geometry.mrao.cam.ac.uk/wp-content/uploads/2015/02/BlackHole.pdf22 Feb 2015: Black Holes 2002 24. Vertex Factor II• Evaluate the second order diagram.
Search history
Recently clicked results
Recently clicked results
Your click history is empty.
Recent searches
- watson |u:people.ast.cam.ac.uk (1) · moments ago
Recent searches
Your search history is empty.