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Thomas Larsson
Apr27-04, 01:45 PM
<jabberwocky><div class="vbmenu_control"><a href="jabberwocky:;" onClick="newWindow=window.open('','usenetCode','toolbar=no, location=no,scrollbars=yes,resizable=yes,status=no ,width=650,height=400'); newWindow.document.write('<HTML><HEAD><TITLE>Usenet ASCII</TITLE></HEAD><BODY topmargin=0 leftmargin=0 BGCOLOR=#F1F1F1><table border=0 width=625><td bgcolor=midnightblue><font color=#F1F1F1>This Usenet message\'s original ASCII form: </font></td></tr><tr><td width=449><br><br><font face=courier><UL><PRE>Urs Schreiber &lt;Urs.Schreiber@uni-essen.de&gt; wrote in message news:&lt;Pine.LNX.4.31.0404220635180.32710-100000@feynman.harvard.edu&gt;...\n\nI really don\'t feel comfortable with posting to sps, so I prefer to\nmove this discussion to neutral territory.\n\n&gt; On Tue, 20 Apr 2004, Thomas Larsson wrote:\n&gt; &gt; My point was that these extensions are not part of string theory,\n&gt; &gt; because if they were, GSW should have known about them.\n&gt;\n&gt; I think the point is that anomalies due to chiral fermions can be seen\n&gt; already in the low energy effective action, so that we can say something\n&gt; about them without knowing the full effective action/closed string field\n&gt; theory.\n\nThe problem is that the Virasoro-like anomalies are functionals of a\nprivileged 1D curve, which can naturally interpreted as the observer\'s\ntrajectory. There is no way to see such an anomaly in a formalism where\nthe observer, or at least her trajectory, is not explicitly present.\nThis is the case in field and string theory. Lubos Motl is of course\nperfectly right when he says that GSW know all about the diff anomalies\nthat can arise in string theory. The Virasoro-like anomalies can not.\n\nHowever, I noted that Damour-Henneaux-Nicolai implicitly introduce what\nI call the observer\'s position. More about that below.\n\n&gt; &gt; A finite truncation of a graded Lie algebra violates the Jacobi identities,\n&gt; &gt; no? E.g., if we have A, B in g_1 and C in g_-1, [[A,B],C] is in g_1 so it\n&gt; &gt; should not be truncated, but it is because [A,B] is in g_2.\n&gt;\n&gt; Sorry for expressing myself badly. What can be truncated is the expansion\n&gt; of the sigma-model dynamics on the E10/K(E10) group. This truncation\n&gt; is consistent in the sense of a perturbative truncation at some given\n&gt; order is consistent in that higher order terms won\'t invalidate the\n&gt; approximate result at lower order.\n&gt;\n&gt; Of course you are perfectly right that there is no subalgebra of\n&gt; a graded Lie algebra beyond level 0. But the truncation that I\n&gt; was referring to is based on the fact that all elements of E10\n&gt; (or any other KM algebra) at a given level transform under the\n&gt; action of the level-0 subalgebra. Therefore every level can be\n&gt; "understood" by decomposing it into irreps of the level-0\n&gt; subalgebra.\n\nIOW, E10 admits a grading with g_0 = gl(10), all g_k are\nfinite-dimensional g_0 modules, and you can compute g_-k recursively up\nto any fixed order, say 30. Yes, I am pretty sure that this is true,\nand it is an useful description of E10. You can probably do the same\nwith any KM algebra which admits a grading such that g_0 is\nfinite-dimensional. You can definitely to it for all finite-dimensional\nLie algebras, where the grading terminates at some finite order. In\nfact, I have listed the nonlinear realizations that correspond to\nremoving one node in the Dynkin diagram. One day I may find the energy\nto put the list on the arxiv.\n\n&gt;\n&gt; In\n&gt;\n&gt; Damour, Henneaux, Nicolai\n&gt; E10 and the \'small tension expansion\' of M Theory\n&gt; hep-th/0207267\n&gt;\n&gt; a grading of E10 is used which is based on the \'exceptional\'\n&gt; root (instead of on the over-extended root, in their\n&gt; nomenclature). This way E10 is decomposed into irreps\n&gt; of its SL(10) subalgebra, level by level.\n\nThis is a cool paper. Something which I wondered about for some time is\nwhy West talks about E11 and you talked about E10. I now realize that\nWest looks for M-theory in 11 spacetime dimensions and DHN works in 10\nspatial dimensions; their sigma-model is formulated in terms of a\ntime-dependent group element V(t) in E10, there is a lapse function,\netc.\n\n&gt; The important\n&gt; point now is that these irreps are of course nothing\n&gt; but tensors, and that these tensors can be identified with\n&gt; spatial modes of tensor fields of the bosonic sector\n&gt; of 11d sugra (namely the metric and the 3-form field).\n\nThe given spatial point x that occurs in (12) of DHN is what I call\nthe observer\'s position, since the fields are "observed" from this\npoint. However, I allow the privileged point to vary with t, so I get a\ntrajectory x(t) (q(t) in my notation).\n\n&gt;\n&gt; So while the configuration point traces out a trajectory\n&gt; on the E10/K(E10) \'manifold\' we can, even lacking a complete\n&gt; understanding of what this full group really is, understand\n&gt; the sugra configuration that this trajectory describes\n&gt; order by order in the above notion of level (which corresponds\n&gt; to an expansion in terms of spatial gradients on the\n&gt; sugra side).\n\nOK, I understand that the geodesic Lagrangian on E10 is well-defined,\nand that it contains the field content of SUGRA plus much more.\nHowever, there are many questions, e.g.\n\n1. What so special about E10? You could almost surely repeat the same\nanalysis for any KM algebra, at least if it has a grading by finite-\ndimensional subspaces. This is true for infinitely many KM algebras, e.g.\n\n*\n|\no-o-o-o-o-...-o-o-o-o- ... -o-o-o-o-o\n\nWhat\'s wrong with these models? If you truncate the grading after finitely\nmany terms, the geodesic Lagrangian depends on finitely many dofs, i.e.\nyou have a quantum mechanics problem. There shouldn\'t be any difficulties\nhere. Whether nasty infinitites arise in the limit that you lift the\ntrunction is probably an open question.\n\n2. Diffeomorphisms! E10 is a fancy generalization of the gl(10) subalgebra\nof the diffeo algebra vect(10), but the remaining diffeos do not seem to\nfit in. In fact, not even translations seem to fit into E10. West seems\nto add translations outside E8; that\'s the P_a in (4.1) of hep-th/0104081.\nYou really need to include all diffeos, essentially for the same reason\nthat you need to go from SUSY to SUGRA. So you need some Lie algebra\nthat contains both E10 and vect(10) as subalgebras, such that their gl(10)\nsubalgebras are identified. Such algebras exist, but if E10 is BIG, they\nare GARGANTUAN.\n\n3. Let us assume that we manage to make the E10 symmetry local, i.e. we\ninclude diffeos in some way. Then vect(10) acts on the graded subspaces\nin some way. In particular, the spatial gradients in (13) of DHN, which\ntransform as symmetric n-tensors under gl(10), must transform as Taylor\ncoefficients, or n-jets, under vect(10). This means that they are\nmultiplied by matrices which depend on the base point x, and that x\nitself transforms non-trivially; for explicit formulas in multi-index\nnotation, see (4.1) of math-ph/9810003. It is not clear to me that\ninfinite towers in (13) really transform as jets.\n\n4. The Lagrangian (4) of DHN depends on the standard invariant bilinear\nform &lt;.|.&gt; on the KM algebra. However, there is no such form if you\ninclude arbitrary diffeos; if there were, you could use it to identify\nthe adjoint and coadjoint reps which are inequivalent. So how can the\ngeodesic Lagrangian be defined in the presence of diffeos?\n\n5. The experimental connection! 11D SUGRA is already on very shaky\nground, since there is virtually no experimental evidence for neither\nSUSY nor extra dimensions. To postulate an infinite, and exponentially\ngrowing, tower of new particles in this situation seems to me a bit bold,\nto put it mildly.\n\n</UL></PRE></font></td></tr></table></BODY><HTML>');"> <IMG SRC=/images/buttons/ip.gif BORDER=0 ALIGN=CENTER ALT="View this Usenet post in original ASCII form">&nbsp;&nbsp;View this Usenet post in original ASCII form </a></div><P></jabberwocky>Urs Schreiber <Urs.Schreiber@uni-essen.de> wrote in message news:<Pine.LNX.4.31.0404220635180.32710-100000@feynman.harvard.edu>...

I really don't feel comfortable with posting to sps, so I prefer to
move this discussion to neutral territory.

> On Tue, 20 Apr 2004, Thomas Larsson wrote:
> > My point was that these extensions are not part of string theory,
> > because if they were, GSW should have known about them.
>
> I think the point is that anomalies due to chiral fermions can be seen
> already in the low energy effective action, so that we can say something
> about them without knowing the full effective action/closed string field
> theory.

The problem is that the Virasoro-like anomalies are functionals of a
privileged 1D curve, which can naturally interpreted as the observer's
trajectory. There is no way to see such an anomaly in a formalism where
the observer, or at least her trajectory, is not explicitly present.
This is the case in field and string theory. Lubos Motl is of course
perfectly right when he says that GSW know all about the diff anomalies
that can arise in string theory. The Virasoro-like anomalies can not.

However, I noted that Damour-Henneaux-Nicolai implicitly introduce what
I call the observer's position. More about that below.

> > A finite truncation of a graded Lie algebra violates the Jacobi identities,
> > no? E.g., if we have A, B in g_1 and C in g_-1, [[A,B],C] is in g_1 so it
> > should not be truncated, but it is because [A,B] is in g_2.
>
> Sorry for expressing myself badly. What can be truncated is the expansion
> of the \sigma-model dynamics on the E10/K(E10) group. This truncation
> is consistent in the sense of a perturbative truncation at some given
> order is consistent in that higher order terms won't invalidate the
> approximate result at lower order.
>
> Of course you are perfectly right that there is no subalgebra of
> a graded Lie algebra beyond level . But the truncation that I
> was referring to is based on the fact that all elements of E10
> (or any other KM algebra) at a given level transform under the
> action of the level-0 subalgebra. Therefore every level can be
> "understood" by decomposing it into irreps of the level-0
> subalgebra.

IOW, E10 admits a grading with g_0 = gl(10), all g_k are
finite-dimensional g_0 modules, and you can compute g_-k recursively up
to any fixed order, say 30. Yes, I am pretty sure that this is true,
and it is an useful description of E10. You can probably do the same
with any KM algebra which admits a grading such that g_0 is
finite-dimensional. You can definitely to it for all finite-dimensional
Lie algebras, where the grading terminates at some finite order. In
fact, I have listed the nonlinear realizations that correspond to
removing one node in the Dynkin diagram. One day I may find the energy
to put the list on the arxiv.

>
> In
>
> Damour, Henneaux, Nicolai
> E10 and the 'small tension expansion' of M Theory
> http://www.arxiv.org/abs/hep-th/0207267
>
> a grading of E10 is used which is based on the 'exceptional'
> root (instead of on the over-extended root, in their
> nomenclature). This way E10 is decomposed into irreps
> of its SL(10) subalgebra, level by level.

This is a cool paper. Something which I wondered about for some time is
why West talks about E11 and you talked about E10. I now realize that
West looks for M-theory in 11 spacetime dimensions and DHN works in 10
spatial dimensions; their \sigma-model is formulated in terms of a
time-dependent group element V(t) in E10, there is a lapse function,
etc.

> The important
> point now is that these irreps are of course nothing
> but tensors, and that these tensors can be identified with
> spatial modes of tensor fields of the bosonic sector
> of 11d sugra (namely the metric and the 3-form field).

The given spatial point x that occurs in (12) of DHN is what I call
the observer's position, since the fields are "observed" from this
point. However, I allow the privileged point to vary with t, so I get a
trajectory x(t) (q(t) in my notation).

>
> So while the configuration point traces out a trajectory
> on the E10/K(E10) 'manifold' we can, even lacking a complete
> understanding of what this full group really is, understand
> the sugra configuration that this trajectory describes
> order by order in the above notion of level (which corresponds
> to an expansion in terms of spatial gradients on the
> sugra side).

OK, I understand that the geodesic Lagrangian on E10 is well-defined,
and that it contains the field content of SUGRA plus much more.
However, there are many questions, e.g.

1. What so special about E10? You could almost surely repeat the same
analysis for any KM algebra, at least if it has a grading by finite-
dimensional subspaces. This is true for infinitely many KM algebras, e.g.

*
|
o-o-o-o-o-...-o-o-o-o- ... -o-o-o-o-o

What's wrong with these models? If you truncate the grading after finitely
many terms, the geodesic Lagrangian depends on finitely many dofs, i.e.
you have a quantum mechanics problem. There shouldn't be any difficulties
here. Whether nasty infinitites arise in the limit that you lift the
trunction is probably an open question.

2. Diffeomorphisms! E10 is a fancy generalization of the gl(10) subalgebra
of the diffeo algebra vect(10), but the remaining diffeos do not seem to
fit in. In fact, not even translations seem to fit into E10. West seems
to add translations outside E8; that's the P_a in (4.1) of http://www.arxiv.org/abs/hep-th/0104081.
You really need to include all diffeos, essentially for the same reason
that you need to go from SUSY to SUGRA. So you need some Lie algebra
that contains both E10 and vect(10) as subalgebras, such that their gl(10)
subalgebras are identified. Such algebras exist, but if E10 is BIG, they
are GARGANTUAN.

3. Let us assume that we manage to make the E10 symmetry local, i.e. we
include diffeos in some way. Then vect(10) acts on the graded subspaces
in some way. In particular, the spatial gradients in (13) of DHN, which
transform as symmetric n-tensors under gl(10), must transform as Taylor
coefficients, or n-jets, under vect(10). This means that they are
multiplied by matrices which depend on the base point x, and that x
itself transforms non-trivially; for explicit formulas in multi-index
notation, see (4.1) of http://www.arxiv.org/abs/math-ph/9810003. It is not clear to me that
infinite towers in (13) really transform as jets.

4. The Lagrangian (4) of DHN depends on the standard invariant bilinear
form <.|.> on the KM algebra. However, there is no such form if you
include arbitrary diffeos; if there were, you could use it to identify
the adjoint and coadjoint reps which are inequivalent. So how can the
geodesic Lagrangian be defined in the presence of diffeos?

5. The experimental connection! 11D SUGRA is already on very shaky
ground, since there is virtually no experimental evidence for neither
SUSY nor extra dimensions. To postulate an infinite, and exponentially
growing, tower of new particles in this situation seems to me a bit bold,
to put it mildly.

Urs Schreiber
Apr28-04, 03:51 AM
<jabberwocky><div class="vbmenu_control"><a href="jabberwocky:;" onClick="newWindow=window.open('','usenetCode','toolbar=no, location=no,scrollbars=yes,resizable=yes,status=no ,width=650,height=400'); newWindow.document.write('<HTML><HEAD><TITLE>Usenet ASCII</TITLE></HEAD><BODY topmargin=0 leftmargin=0 BGCOLOR=#F1F1F1><table border=0 width=625><td bgcolor=midnightblue><font color=#F1F1F1>This Usenet message\'s original ASCII form: </font></td></tr><tr><td width=449><br><br><font face=courier><UL><PRE>\n(BTW, I do know that there is a typo in the subject header. ;-) But I leave\nit the way it is in order not to confuse Google too much.)\n\n"Thomas Larsson" &lt;thomas_larsson_01@hotmail.com&gt; schrieb im Newsbeitrag\nnews:24a23f36.0404240558.79010b23@pos ting.google.com...\n\n&gt; &gt;However, I noted that Damour-Henneaux-Nicolai implicitly introduce what\n&gt; &gt;I call the observer\'s position. More about that below.\n\nTrue. That\'s indeed reminiscent of your approach. For people used to\nhomogeneous cosmologies this step away from descriptions of the "whole\nuniverse" to asymptotically causally disconnected patches near a singularity\nis kind of remarkable. The formulas (to first order) don\'t change, but the\ninterpretation does significantly.\n\n&gt; &gt;IOW, E10 admits a grading with g_0 = gl(10), all g_k are\n&gt; &gt;finite-dimensional g_0 modules, and you can compute g_-k recursively up\n&gt; &gt;to any fixed order, say 30.\n\nYes, and IIRC one can find geodesics in the "group" which run only inside\nthe\nsubspace generated by elements up to a given fixed order.\n\n&gt; &gt;This is a cool paper. Something which I wondered about for some time is\n&gt; &gt;why West talks about E11 and you talked about E10. I now realize that\n&gt; &gt;West looks for M-theory in 11 spacetime dimensions and DHN works in 10\n&gt; &gt;spatial dimensions; their sigma-model is formulated in terms of a\n&gt; &gt;time-dependent group element V(t) in E10, there is a lapse function,\n&gt; &gt;etc.\n\nYou are\nperfectly right that the 10 in E10 comes from the 10 spatial dimensions in\n11d\nsugra. In cosmologist\'s terms the group of E10 is something like the\nultimate\nmidi superspace (space of modes of the spatial geormery) of 11d sugra.\n\nI had a quick look at West\'s paper but so far wasn\'t able to extract an\nanalogous statement for the role played by E11 in his approach. Maybe we\'d\nhave a 0+0 dimensional sigma model in exp(E_11)??\n\n&gt; &gt;The given spatial point x that occurs in (12) of DHN is what I call\n&gt; &gt;the observer\'s position, since the fields are "observed" from this\n&gt; &gt;point. However, I allow the privileged point to vary with t, so I get a\n&gt; &gt;trajectory x(t) (q(t) in my notation).\n\nOk. I think the x in DHN\'s approach is temporally constant, i.e. "comoving".\nBut this is also due to the fact that they initilly choose coordinates such\nthat the spatial shift functions N^i vanish. So I think they partially fix\nthe\ndiff symmetry of the problem before turning the crank.\n\n&gt; &gt;1. What so special about E10? You could almost surely repeat the same\n&gt; &gt;analysis for any KM algebra, at least if it has a grading by finite-\n&gt; &gt;dimensional subspaces. This is true for infinitely many KM algebras, e.g.\n&gt; &gt;\n&gt; &gt; *\n&gt; &gt; |\n&gt; &gt; o-o-o-o-o-...-o-o-o-o- ... -o-o-o-o-o\n&gt; &gt;\n&gt; &gt;What\'s wrong with these models? If you truncate the grading after\nfinitely\n&gt; &gt;many terms, the geodesic Lagrangian depends on finitely many dofs, i.e.\n&gt; &gt;you have a quantum mechanics problem. There shouldn\'t be any difficulties\n&gt; &gt;here. Whether nasty infinitites arise in the limit that you lift the\n&gt; &gt;trunction is probably an open question.\n\nYes. Indeed DHN discuss that you can get KM algebras describing the billiard\nlimit of all kinds of gravitational theories. Apparently pure d+1\ndimensional\ngravity corresponds to the KM algebra AE_d . See pp. 57 for a detailed\ndiscussion of the d=3 case.\n\nBut, maybe surprisingly, 11d sugra is special in that only here does one\nknow a consistent interpretation of the objects in the KM sigma-model away\nfrom the billiard limit in terms of spatial gradients of fields of the\ngravitational theory.\n\nOn p. 68 of hep-th/0212256 it says:\n\n"Similarly, one would like to associate the generators [the elements of the\ngiven KM algebra] with higher order spatial gradients. However, the proper\nphysical interpretation of these fields as well as of the other higher level\ncomponents remains yet to be found.\n\n"In the case of the relation between supergravity in D=11 and the E_10 coset\nmodel one could pursue the correspondence between spacetime fields and coset\ncoordinates up to the gl(10,R) level l=3 included (corresponding to height\n29). The correspondence worked thanks to several "miraculous" agreements\nbetween the numerical coefficients appearing in both Lagrangians."\n\nIt seems that for E_10 also the KM elements which do not correspond to SUGRA\ndegrees of freedom can be consistently identified. At least some evidence\nfor the identification of "imaginary" root elements in E_10 with D-branes is\ngiven in\n\nBrown, Ganor, Helfgott:\nM-theory and E_10: Billiards, Branes, and Imaginary Roots\nhep-th/0401053\n\nTherein also the quantization of the sigma model is discussed and\nnon-trivial tests of the quantization are claimed to be consistent with the\nknown mass spectrum of the branes.\n\n(BTW, I am not sure that I understand the origin of the linear term in the\nlowest order part of the E_10 Laplacian in equation (38). )\n\n&gt; &gt;2. Diffeomorphisms! E10 is a fancy generalization of the gl(10)\nsubalgebra\n&gt; &gt;of the diffeo algebra vect(10), but the remaining diffeos do not seem to\n&gt; &gt;fit in.\n\nSeems to me that diffeos would appear at best very indirectly in the DHN\nframework, since everything is expanded about that arbitrary but fixed point\nx.\n\n&gt; &gt;You really need to include all diffeos, essentially for the same reason\n&gt; &gt;that you need to go from SUSY to SUGRA.\n\nI am not sure what you are trying to argue here. DHN demonstrate that the\nE_10 sigma model reproduces SUGRA. So why would they need to add something\nto\ndo the same?\n\nI can see why you would expect diffeos to be included explicitly. But I\nthink\nthe fact that the equations of motion of SUGRA are reproduced by E_10 shows\nthat the\nsystem must know about the diffeos already in some sense. Otherwise it\ncouldn\'t yield gravity.\n\n&gt; &gt;3. Let us assume that we manage to make the E10 symmetry local,\n\nSeems to me that you are beginning to think of exp(E_10) in some other\napplication\nthan as the target space of a 1+0 dim sigma model. Namely in that context\nthere is no sense in which you clould make E10 local. It is already local on\nthe worldline, trivially.\n\n&gt; &gt;5. The experimental connection! 11D SUGRA is already on very shaky\n&gt; &gt;ground, since there is virtually no experimental evidence for neither\n&gt; &gt;SUSY nor extra dimensions. To postulate an infinite, and exponentially\n&gt; &gt;growing, tower of new particles in this situation seems to me a bit bold,\n&gt; &gt;to put it mildly.\n\nAs I said above, to lowest order all this works for pure/non-pure gravity in\nany number of dimensions. But apparently the bosonic sector of 11d sugra is\nspecial\nin that here the match with the KM sigma model works also for (all?) higher\norders.\n\nLet me summarize the line of reasoning which leads to 11D sugra this way\nwithout even mentioning strings or M-theory:\n\n- Write down a gravitational Lagrangian possibly with form field matter and\ndilatons in any number d+1 of dimensions.\n\n- Go to the limit close to a spacelike singularity. Here the spacetime\npoints always "decouple" and one is left with a billiard motion in\nconfiguration space.\n\n- In some cases the billiard walls happen to be form Weyl chamber of some KM\nalgebra, with the logarithms of the metric scale factors interpreted as\ncoordinates in the Cartan subalgebra.\n\n- In these cases the billiard motion can be identified with some lowest\norder approximation of geodesic motion on exp(KM).\n\n- Now we _guess_ that hence the full geodesic motion on this exp(KM) might\ndescribe the full original gravitational theory.\n\n- When we check this guess, it turns out to work only for 11D SUGRA and\nKM=E_10. In this case we find that 11d sugra is a *subset* of the dynamics\ncontained in the geodesic motion on exp(E_10).\n\nInteresting, isn\'t it?\n\n</UL></PRE></font></td></tr></table></BODY><HTML>');"> <IMG SRC=/images/buttons/ip.gif BORDER=0 ALIGN=CENTER ALT="View this Usenet post in original ASCII form">&nbsp;&nbsp;View this Usenet post in original ASCII form </a></div><P></jabberwocky>(BTW, I do know that there is a typo in the subject header. ;-) But I leave
it the way it is in order not to confuse Google too much.)

"Thomas Larsson" <thomas_larsson_01@hotmail.com> schrieb im Newsbeitrag
news:24a23f36.0404240558.79010b23@posting.google.c om...

> >However, I noted that Damour-Henneaux-Nicolai implicitly introduce what
> >I call the observer's position. More about that below.

True. That's indeed reminiscent of your approach. For people used to
homogeneous cosmologies this step away from descriptions of the "whole
universe" to asymptotically causally disconnected patches near a singularity
is kind of remarkable. The formulas (to first order) don't change, but the
interpretation does significantly.

> >IOW, E10 admits a grading with g_0 = gl(10), all g_k are
> >finite-dimensional g_0 modules, and you can compute g_-k recursively up
> >to any fixed order, say 30.

Yes, and IIRC one can find geodesics in the "group" which run only inside
the
subspace generated by elements up to a given fixed order.

> >This is a cool paper. Something which I wondered about for some time is
> >why West talks about E11 and you talked about E10. I now realize that
> >West looks for M-theory in 11 spacetime dimensions and DHN works in 10
> >spatial dimensions; their \sigma-model is formulated in terms of a
> >time-dependent group element V(t) in E10, there is a lapse function,
> >etc.

You are
perfectly right that the 10 in E10 comes from the 10 spatial dimensions in
11d
sugra. In cosmologist's terms the group of E10 is something like the
ultimate
midi superspace (space of modes of the spatial geormery) of 11d sugra.

I had a quick look at West's paper but so far wasn't able to extract an
analogous statement for the role played by E11 in his approach. Maybe we'd
have a 0+0 dimensional \sigma model in \exp(E_{11})??

> >The given spatial point x that occurs in (12) of DHN is what I call
> >the observer's position, since the fields are "observed" from this
> >point. However, I allow the privileged point to vary with t, so I get a
> >trajectory x(t) (q(t) in my notation).

Ok. I think the x in DHN's approach is temporally constant, i.e. "comoving".
But this is also due to the fact that they initilly choose coordinates such
that the spatial shift functions N^i vanish. So I think they partially fix
the
diff symmetry of the problem before turning the crank.

> >1. What so special about E10? You could almost surely repeat the same
> >analysis for any KM algebra, at least if it has a grading by finite-
> >dimensional subspaces. This is true for infinitely many KM algebras, e.g.
> >
> > *
> > |
> > o-o-o-o-o-...-o-o-o-o- ... -o-o-o-o-o
> >
> >What's wrong with these models? If you truncate the grading after
finitely
> >many terms, the geodesic Lagrangian depends on finitely many dofs, i.e.
> >you have a quantum mechanics problem. There shouldn't be any difficulties
> >here. Whether nasty infinitites arise in the limit that you lift the
> >trunction is probably an open question.

Yes. Indeed DHN discuss that you can get KM algebras describing the billiard
limit of all kinds of gravitational theories. Apparently pure d+1
dimensional
gravity corresponds to the KM algebra AE_d . See pp. 57 for a detailed
discussion of the d=3 case.

But, maybe surprisingly, 11d sugra is special in that only here does one
know a consistent interpretation of the objects in the KM \sigma-model away
from the billiard limit in terms of spatial gradients of fields of the
gravitational theory.

On p. 68 of http://www.arxiv.org/abs/hep-th/0212256 it says:

"Similarly, one would like to associate the generators [the elements of the
given KM algebra] with higher order spatial gradients. However, the proper
physical interpretation of these fields as well as of the other higher level
components remains yet to be found.

"In the case of the relation between supergravity in D=11 and the E_{10} coset
model one could pursue the correspondence between spacetime fields and coset
coordinates up to the gl(10,R) level l=3 included (corresponding to height
29). The correspondence worked thanks to several "miraculous" agreements
between the numerical coefficients appearing in both Lagrangians."

It seems that for E_{10} also the KM elements which do not correspond to SUGRA
degrees of freedom can be consistently identified. At least some evidence
for the identification of "imaginary" root elements in E_{10} with D-branes is
given in

Brown, Ganor, Helfgott:
M-theory and E_{10}: Billiards, Branes, and Imaginary Roots
http://www.arxiv.org/abs/hep-th/0401053

Therein also the quantization of the \sigma model is discussed and
non-trivial tests of the quantization are claimed to be consistent with the
known mass spectrum of the branes.

(BTW, I am not sure that I understand the origin of the linear term in the
lowest order part of the E_{10} Laplacian in equation (38). )

> >2. Diffeomorphisms! E10 is a fancy generalization of the gl(10)
subalgebra
> >of the diffeo algebra vect(10), but the remaining diffeos do not seem to
> >fit in.

Seems to me that diffeos would appear at best very indirectly in the DHN
framework, since everything is expanded about that arbitrary but fixed point
x.

> >You really need to include all diffeos, essentially for the same reason
> >that you need to go from SUSY to SUGRA.

I am not sure what you are trying to argue here. DHN demonstrate that the
E_{10} \sigma model reproduces SUGRA. So why would they need to add something
to
do the same?

I can see why you would expect diffeos to be included explicitly. But I
think
the fact that the equations of motion of SUGRA are reproduced by E_{10} shows
that the
system must know about the diffeos already in some sense. Otherwise it
couldn't yield gravity.

> >3. Let us assume that we manage to make the E10 symmetry local,

Seems to me that you are beginning to think of \exp(E_{10}) in some other
application
than as the target space of a 1+0 dim \sigma model. Namely in that context
there is no sense in which you clould make E10 local. It is already local on
the worldline, trivially.

> >5. The experimental connection! 11D SUGRA is already on very shaky
> >ground, since there is virtually no experimental evidence for neither
> >SUSY nor extra dimensions. To postulate an infinite, and exponentially
> >growing, tower of new particles in this situation seems to me a bit bold,
> >to put it mildly.

As I said above, to lowest order all this works for pure/non-pure gravity in
any number of dimensions. But apparently the bosonic sector of 11d sugra is
special
in that here the match with the KM \sigma model works also for (all?) higher
orders.

Let me summarize the line of reasoning which leads to 11D sugra this way
without even mentioning strings or M-theory:

- Write down a gravitational Lagrangian possibly with form field matter and
dilatons in any number d+1 of dimensions.

- Go[/itex] to the limit close to a spacelike singularity. Here the spacetime
points always "decouple" and one is left with a billiard motion in
configuration space.

- In some cases the billiard walls happen to be form Weyl chamber of some KM
algebra, with the logarithms of the metric scale factors interpreted as
coordinates in the Cartan subalgebra.

- In these cases the billiard motion can be identified with some lowest
order approximation of geodesic motion on \exp(KM).

- Now we _guess_ that hence the full geodesic motion on this \exp(KM) might
describe the full original gravitational theory.

- When we check this guess, it turns out to work only for 11D SUGRA and
KM=E_{10}. In this case we find that 11d sugra is a *subset* of the dynamics
contained in the geodesic motion on [itex]\exp(E_{10}).

Interesting, isn't it?

Thomas Larsson
Apr28-04, 02:27 PM
<jabberwocky><div class="vbmenu_control"><a href="jabberwocky:;" onClick="newWindow=window.open('','usenetCode','toolbar=no, location=no,scrollbars=yes,resizable=yes,status=no ,width=650,height=400'); newWindow.document.write('<HTML><HEAD><TITLE>Usenet ASCII</TITLE></HEAD><BODY topmargin=0 leftmargin=0 BGCOLOR=#F1F1F1><table border=0 width=625><td bgcolor=midnightblue><font color=#F1F1F1>This Usenet message\'s original ASCII form: </font></td></tr><tr><td width=449><br><br><font face=courier><UL><PRE>Urs Schreiber &lt;Urs.Schreiber@uni-essen.de&gt; skrev i\ndiskussionsgruppsmeddelandet:408f70af\\$1@news. sentex.net...\n\n&gt; I am not sure what you are trying to argue here. DHN demonstrate that the\n&gt; E_10 sigma model reproduces SUGRA. So why would they need to add something\n&gt; to\n&gt; do the same?\n\nLet me come back to West\'s work, which I understand better. There is\nevidently a relation to DHN, but exactly how it works is not clear to\nme, and judging from the discussion in the introduction of\nhep-th/0312247 it is not completely clear to the specialists either.\n\nAnyway, in hep-th/0005270 West proves that 11D sugra can be written as\na non-linear realization of the group G11, with generators K^a_b\n(GL(11)), P_a (translations), R^abc (3-form) and R^abcdef (6-form),\nsee (2.7-8). G11 minus translations can be identified with the level\n0, -1 and -2 subspaces of E11, which is the basis for the E11\nconjecture.\n\nHowever, he writes on page 6 that we must find a non-linear\nrealization of the closure of this group with the conformal group.\nThis closure is a bigger group which includes diffeos. This follows\nfrom old work by Ogievetsky [ref. 19, entitled "Infinite-dimensional\nalgebra of general covariance group as the closure of conformal and\nlinear groups", from 1973], which formulated ordinary GR as a\nnon-linear realization. Part of this big algebra, namely the E11\naction on translations, is described in section 3 of hep-th/0307098.\n\nBut one can avoid writing down this big group explicitly by\nconsidering simultaneous reps of G11 and the conformal group, which\ngives you diff invariance indirectly. Only the simulataneously\ninvariant objects in (2.25-26) appear in sugra.\n\nOne may also observe that hep-th/0307098 is mainly concerned with\nextending the results to susy, discussed already in hep-th/0005270.\nWest finds a GL(32) which he argues is a subgroup of the "M-algebra"\nOsp(1/64).\n\n&gt; I can see why you would expect diffeos to be included explicitly. But I\n&gt; think\n&gt; the fact that the equations of motion of SUGRA are reproduced by E_10 shows\n&gt; that the\n&gt; system must know about the diffeos already in some sense. Otherwise it\n&gt; couldn\'t yield gravity.\n\nHm. On second thought, I am pretty sure that vect(10) is not a\nsubalgebra of E10, so if DHN claim that, they must be wrong.\nProof (almost): Assume the opposite. Any Kac-Moody algebra carries a\nsymmetric, bilinear, invariant form &lt;.|.&gt;. This equips vect(10) with\nsuch a form by restriction, but it is known that vect(10) does not\nhave such a form. So the only possibility is that the restriction is\nidentically zero. However, if further restriction to gl(10) gives us\nthe standard form &lt;h^a_b, h^c_d&gt; = delta^a_d delta^c_b != 0, which I\nbelieve it should do, then we have a contradiction. QED.\n\n&gt; Interesting, isn\'t it?\n&gt;\n\nJudging by the number of papers on E10, E11 and nonlinear realizations\nover the last few weeks, this is a hot topic. I agree that nonlinear\nrealizations are very interesting, and appears that all kinds of\nsugra and string theories can be formulated in this way, at least the\nbosonic part.\n\nThis raises the question how general this method is. Can you associate\none (or several) interesting models with every grading of every Lie\nalgebra and superalgebra, or are there any restrictions? It seems like\na potential treasure chest for prospective model builders.\n\nAnother interesting question is whether the standard model can be\nformulated as a nonlinear realization, or if there is some tight\nextension that can. From Ogievetsky\'s work we know that GR can. This\nquestion should be of interest both for string theorists working\ntop-down from some 11D M-theory, and for us infidels who hope that\nthere might be some economic 4D way to make the SM beautiful.\n\nWhether or not E10 and E11 are relevant remains to be seen. West\nproved the importance of G11 and that is a subalgebra of E11. If we\nbelieve in the existence of some hugely symmetric theory, and that the\nsymmetry is a Kac-Moody algebra, then we are apparently forced to E11.\nBut is this belief right? One can construct interesting algebras\ncontaining G11 which are not KM algebras because they don\'t have a\nCartan matrix. E.g., the Cartan prolong is the biggest graded\nsubalgebra of vect(627) with g_-2 = R^abcdef, g_-1 = R^abc, and\ng_0 = K^a_b. This algebra contains G11 but I don\'t know if it contains\nanything more; one must check.\n\n</UL></PRE></font></td></tr></table></BODY><HTML>');"> <IMG SRC=/images/buttons/ip.gif BORDER=0 ALIGN=CENTER ALT="View this Usenet post in original ASCII form">&nbsp;&nbsp;View this Usenet post in original ASCII form </a></div><P></jabberwocky>Urs Schreiber <Urs.Schreiber@uni-essen.de> skrev i
diskussionsgruppsmeddelandet:408f70af$1@news.sente x.net...

> I am not sure what you are trying to argue here. DHN demonstrate that the
> E_{10} \sigma model reproduces SUGRA. So why would they need to add something
> to
> do the same?

Let me come back to West's work, which I understand better. There is
evidently a relation to DHN, but exactly how it works is not clear to
me, and judging from the discussion in the introduction of
http://www.arxiv.org/abs/hep-th/0312247 it is not completely clear to the specialists either.

Anyway, in http://www.arxiv.org/abs/hep-th/0005270 West proves that 11D sugra can be written as
a non-linear realization of the group G11, with generators K^{a_b}(GL(11)), P_a (translations), R^{abc} (3-form) and R^{abcdef} (6-form),
see (2.7-8). G11 minus translations can be identified with the level
0, -1 and -2 subspaces of E11, which is the basis for the E11
conjecture.

However, he writes on page 6 that we must find a non-linear
realization of the closure of this group with the conformal group.
This closure is a bigger group which includes diffeos. This follows
from old work by Ogievetsky [ref. 19, entitled "Infinite-dimensional
algebra of general covariance group as the closure of conformal and
linear groups", from 1973], which formulated ordinary GR as a
non-linear realization. Part of this big algebra, namely the E11
action on translations, is described in section 3 of http://www.arxiv.org/abs/hep-th/0307098.

But one can avoid writing down this big group explicitly by
considering simultaneous reps of G11 and the conformal group, which
gives you diff invariance indirectly. Only the simulataneously
invariant objects in (2.25-26) appear in sugra.

One may also observe that http://www.arxiv.org/abs/hep-th/0307098 is mainly concerned with
extending the results to susy, discussed already in http://www.arxiv.org/abs/hep-th/0005270.
West finds a GL(32) which he argues is a subgroup of the "M-algebra"
Osp(1/64).

> I can see why you would expect diffeos to be included explicitly. But I
> think
> the fact that the equations of motion of SUGRA are reproduced by E_{10} shows
> that the
> system must know about the diffeos already in some sense. Otherwise it
> couldn't yield gravity.

Hm. On second thought, I am pretty sure that vect(10) is not a
subalgebra of E10, so if DHN claim that, they must be wrong.
Proof (almost): Assume the opposite. Any Kac-Moody algebra carries a
symmetric, bilinear, invariant form <.|.>. This equips vect(10) with
such a form by restriction, but it is known that vect(10) does not
have such a form. So the only possibility is that the restriction is
identically zero. However, if further restriction to gl(10) gives us
the standard form <h^{a_b}, h^{c_d}> = \delta^a_d \delta^c_b != 0, which I
believe it should do, then we have a contradiction. QED.

> Interesting, isn't it?
>

Judging by the number of papers on E10, E11 and nonlinear realizations
over the last few weeks, this is a hot topic. I agree that nonlinear
realizations are very interesting, and appears that all kinds of
sugra and string theories can be formulated in this way, at least the
bosonic part.

This raises the question how general this method is. Can you associate
one (or several) interesting models with every grading of every Lie
algebra and superalgebra, or are there any restrictions? It seems like
a potential treasure chest for prospective model builders.

Another interesting question is whether the standard model can be
formulated as a nonlinear realization, or if there is some tight
extension that can. From Ogievetsky's work we know that GR can. This
question should be of interest both for string theorists working
top-down from some 11D M-theory, and for us infidels who hope that
there might be some economic 4D way to make the SM beautiful.

Whether or not E10 and E11 are relevant remains to be seen. West
proved the importance of G11 and that is a subalgebra of E11. If we
believe in the existence of some hugely symmetric theory, and that the
symmetry is a Kac-Moody algebra, then we are apparently forced to E11.
But is this belief right? One can construct interesting algebras
containing G11 which are not KM algebras because they don't have a
Cartan matrix. E.g., the Cartan prolong is the biggest graded
subalgebra of vect(627) with g_-2 = R^{abcdef}, g_-1 = R^{abc}, and
g_0 = K^{a_b}. This algebra contains G11 but I don't know if it contains
anything more; one must check.