The Ghost-propagator DSE - Physics
The Ghost-propagator DSE - Physics
The Ghost-propagator DSE - Physics
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<strong>The</strong> Low-Momentum <strong>Ghost</strong><br />
Dressing Function, the Gluon<br />
Mass and the transition<br />
between Decoupling and<br />
Scaling IR solutions<br />
Based on: JHEP0806(2008)008, PRD80(2009)085018,<br />
PRD82(2010)054007.<br />
by<br />
J. Rodríguez-Quintero;<br />
In collaboration with many other people: A.C. Aguilar, D. Binosi, Ph. Boucaud, M.E.<br />
Gómez, A. Le Yaouanc, J.P. Leroy, J. Micheli, J. Papavassiliou, O. Pène<br />
“T(R)opical QCD”; September 28 th ;Cairns 2010.
Light Cone 2010<br />
Scaling<br />
Vs.<br />
Decoupling
World Cup 2010<br />
Spain<br />
1.- Casillas<br />
4.- S. Ramos<br />
3.- Capdevilla<br />
23.-Piqué<br />
5.- Puyol<br />
8.- Iniesta<br />
10.-Xavi<br />
20.-X. Alonso<br />
22.-Navas<br />
21.-Silva<br />
7.- Villa<br />
Coach: V. Del Bosque<br />
Vs.<br />
1.- Neuer<br />
16.-Lahm<br />
3.- Friedrich<br />
17.-Mertesacker<br />
14.-Badstuber<br />
7.- Schweinsteiger<br />
6.- Khedira<br />
13.-Muller<br />
8.- Ozil<br />
10.-Podolski<br />
11.-Klose<br />
Deutschland<br />
Coach: J. Low
World Cup 2010<br />
Spain<br />
1.- Casillas<br />
4.- S. Ramos<br />
3.- Capdevilla<br />
23.-Piqué<br />
5.- Puyol<br />
8.- Iniesta<br />
10.-Xavi<br />
20.-X. Alonso<br />
22.-Navas<br />
21.-Silva<br />
7.- Villa<br />
Coach: V. Del Bosque<br />
Vs.<br />
1.- Neuer<br />
16.-Lahm<br />
3.- Friedrich<br />
17.-Mertesacker<br />
14.-Badstuber<br />
7.- Schweinsteiger<br />
6.- Khedira<br />
13.-Muller<br />
8.- Ozil<br />
10.-Podolski<br />
11.-Klose<br />
Deutschland<br />
Coach: J. Low
Based on: JHEP0806(2008)008, PRD80(2009)085018,<br />
PRD82(2010)054007.<br />
by<br />
J. Rodríguez-Quintero;<br />
In collaboration with many other people: A.C. Aguilar, D. Binosi, Ph. Boucaud, M.E.<br />
Gómez, A. Le Yaouanc, J.P. Leroy, J. Micheli, J. Papavassiliou, O. Pène<br />
“T(R)opical QCD”; September 28 th ;Cairns 2010.
QCD: SU(3) color interaction<br />
<strong>The</strong> QCD Lagrangian:<br />
Three-gluon interaction Four-gluon interaction<br />
Fadeev-Popov<br />
(ghost felds)<br />
ghost-gluon interaction
QCD: SU(3) color interaction<br />
<strong>The</strong> QCD Lagrangian:<br />
Pure Yang-Mills theory<br />
Three-gluon interaction Four-gluon interaction ghost-gluon interaction
QCD in the IR
QCD in the IR<br />
C'est “chiant” l'IR !!!
QCD in the IR (II)
QCD in the IR (III)
QCD in the IR (III)
Break: UV results
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong> (I)
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong> (I)<br />
where:<br />
All in Landau gauge!!
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong> (I)<br />
where:<br />
All in Landau gauge!!
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong> (II)<br />
After MOM renormalization:<br />
One obtains:
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong> (II)<br />
One obtains:
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong> (II)<br />
One obtains:
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong> (II)<br />
One obtains:
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong> (II)<br />
One obtains:<br />
<strong>The</strong> integral is UV divergent!!
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong> (II)<br />
One obtains:<br />
UV-cutof dependences cancel to each other!!<br />
(in virtue of the interplay of ghost and gluon anomalous dimensions)
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong> (II)<br />
One obtains:<br />
UV-cutof dependences cancel to each other!!<br />
(in virtue of the interplay of ghost and gluon anomalous dimensions)<br />
For not to have to deal with UV, on can subtract:
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong> (II)<br />
One obtains:<br />
UV-cutof dependences cancel to each other!!<br />
(in virtue of the interplay of ghost and gluon anomalous dimensions)<br />
For not to have to deal with UV, on can subtract:<br />
will ultimately go to 0
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong> (II)<br />
One obtains:<br />
UV-cutof dependences cancel to each other!!<br />
(in virtue of the interplay of ghost and gluon anomalous dimensions)<br />
For not to have to deal with UV, on can subtract:<br />
will ultimately go to 0<br />
is positive and non-zero
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong> (III)<br />
will ultimately go to 0<br />
is positive and non-zero
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong> (III)<br />
<strong>The</strong>n:<br />
will ultimately go to 0<br />
is positive and non-zero
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong> (III)<br />
<strong>The</strong>n:<br />
will ultimately go to 0<br />
is positive and non-zero
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong> (III)<br />
<strong>The</strong>n:<br />
will ultimately go to 0<br />
is positive and non-zero
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong> (III)<br />
<strong>The</strong>n:<br />
will ultimately go to 0<br />
is positive and non-zero
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (I)<br />
<strong>The</strong>n:<br />
will ultimately go to 0<br />
is positive and non-zero
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (I)<br />
<strong>The</strong>n:<br />
will ultimately go to 0<br />
is positive and non-zero<br />
while ( )
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (I)<br />
<strong>The</strong>n:<br />
will ultimately go to 0<br />
is positive and non-zero<br />
while ( )
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (I)<br />
<strong>The</strong>n:<br />
will ultimately go to 0<br />
is positive and non-zero<br />
➔<br />
➔
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (I)<br />
<strong>The</strong>n:<br />
will ultimately go to 0<br />
is positive and non-zero<br />
➔<br />
➔
Part II: A new hope
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (II)<br />
<strong>The</strong>n:<br />
will ultimately go to 0<br />
is positive and non-zero
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (II)<br />
<strong>The</strong>n:<br />
will ultimately go to 0<br />
is positive and non-zero<br />
while ( )
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (II)<br />
<strong>The</strong>n:<br />
will ultimately go to 0<br />
is positive and non-zero<br />
while ( )
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (III)<br />
<strong>The</strong>n:<br />
will ultimately go to 0<br />
is positive and non-zero
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (III)<br />
<strong>The</strong>n:<br />
will ultimately go to 0<br />
is positive and non-zero<br />
LQCD favours
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (IV)<br />
In particular:<br />
will ultimately go to 0<br />
is positive and non-zero<br />
Next-to-leading asymptotic approximation:
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (IV)<br />
In particular:<br />
will ultimately go to 0<br />
is positive and non-zero<br />
Next-to-leading asymptotic approximation:<br />
Zero-momentum ghost dressing
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (IV)<br />
In particular:<br />
will ultimately go to 0<br />
is positive and non-zero<br />
Next-to-leading asymptotic approximation:<br />
Zero-momentum ghost dressing<br />
Zero-momentum Taylor-scheme efective charge<br />
A. Aguilar, D. Binosi, J. Papavassiliou, J.R-Q; PRD80(2009)085018
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (IV)<br />
In particular:<br />
will ultimately go to 0<br />
is positive and non-zero<br />
Next-to-leading asymptotic approximation:<br />
Zero-momentum ghost dressing<br />
Zero-momentum Taylor-scheme efective charge<br />
A. Aguilar, D. Binosi, J. Papavassiliou, J.R-Q; PRD80(2009)085018<br />
Zero-momentum gluon mass
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (IV)<br />
In particular:<br />
will ultimately go to 0<br />
is positive and non-zero<br />
Next-to-leading asymptotic approximation:<br />
Zero-momentum ghost dressing<br />
Zero-momentum Taylor-scheme efective charge<br />
A. Aguilar, D. Binosi, J. Papavassiliou, J.R-Q; PRD80(2009)085018<br />
O �q 2 �
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (V)<br />
Next-to-leading asymptotic approximation:<br />
Zero-momentum Taylor-scheme efective charge<br />
A. Aguilar, D. Binosi, J. Papavassiliou, J.R-Q; PRD80(2009)085018<br />
QED-like PT efective charge:<br />
�d �q� = g 2 � ��q 2 � = g 2 ��q 2 �<br />
[1�G �q 2 �] 2
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (V)<br />
Next-to-leading asymptotic approximation:<br />
Zero-momentum Taylor-scheme efective charge<br />
A. Aguilar, D. Binosi, J. Papavassiliou, J.R-Q; PRD80(2009)085018<br />
QED-like PT efective charge:<br />
�d �q� = g 2 � ��q 2 � = g 2 ��q 2 �<br />
[1�G �q 2 �] 2
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (V)<br />
Next-to-leading asymptotic approximation:<br />
Zero-momentum Taylor-scheme efective charge<br />
A. Aguilar, D. Binosi, J. Papavassiliou, J.R-Q; PRD80(2009)085018<br />
QED-like PT efective charge:<br />
�d �q� = g 2 � ��q 2 � = g 2 ��q 2 �<br />
[1�G �q 2 �] 2
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (V)<br />
Next-to-leading asymptotic approximation:<br />
Zero-momentum Taylor-scheme efective charge<br />
A. Aguilar, D. Binosi, J. Papavassiliou, J.R-Q; PRD80(2009)085018<br />
QED-like PT efective charge:<br />
�d �q� = g 2 ��q � 2 g<br />
� = 2 ��q 2 �<br />
[1�G �q 2 �] 2 ≃ �g 2 �q 2 �<br />
q 2<br />
at asymptotically large<br />
momenta!!
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (V)<br />
Next-to-leading asymptotic approximation:<br />
Zero-momentum Taylor-scheme efective charge<br />
A. Aguilar, D. Binosi, J. Papavassiliou, J.R-Q; PRD80(2009)085018<br />
QED-like PT efective charge:<br />
�d �q� = g 2 � ��q 2 � = g 2 ��q 2 �<br />
[1�G �q 2 �] 2 ≃ �g 2 �q 2 �<br />
q 2 �M 2<br />
at low momenta!!
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (V)<br />
Next-to-leading asymptotic approximation:<br />
Zero-momentum Taylor-scheme efective charge<br />
A. Aguilar, D. Binosi, J. Papavassiliou, J.R-Q; PRD80(2009)085018<br />
QED-like PT efective charge:<br />
�d �q� = g 2 � ��q 2 � = g 2 ��q 2 �<br />
[1�G �q 2 �] 2 ≃ �g 2 �q 2 �<br />
q 2 �M 2<br />
IR efective charge!!
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (V)<br />
Next-to-leading asymptotic approximation:<br />
Zero-momentum Taylor-scheme efective charge<br />
A. Aguilar, D. Binosi, J. Papavassiliou, J.R-Q; PRD80(2009)085018<br />
QED-like PT efective charge:<br />
�d �q� = g 2 � ��q 2 � = g 2 ��q 2 �<br />
[1�G �q 2 �] 2 ≃ �g 2 �q 2 �<br />
q 2 �M 2<br />
Taylor efective charge:<br />
2 2 2 2<br />
�r�q� = gT ��q � F �q �<br />
IR efective charge!!
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (V)<br />
Next-to-leading asymptotic approximation:<br />
Zero-momentum Taylor-scheme efective charge<br />
A. Aguilar, D. Binosi, J. Papavassiliou, J.R-Q; PRD80(2009)085018<br />
QED-like PT efective charge:<br />
�d �q� = g 2 � ��q 2 � = g 2 ��q 2 �<br />
[1�G �q 2 �] 2 ≃ �g 2 �q 2 �<br />
q 2 �M 2<br />
Taylor efective charge:<br />
2 2 2 2 2<br />
�r�q� = gT ��q � F �q � = gT ���q 2 2<br />
2<br />
� [1�G �q �] F 2 �q 2 �<br />
IR efective charge!!
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (V)<br />
Next-to-leading asymptotic approximation:<br />
Zero-momentum Taylor-scheme efective charge<br />
A. Aguilar, D. Binosi, J. Papavassiliou, J.R-Q; PRD80(2009)085018<br />
QED-like PT efective charge:<br />
�d �q� = g 2 � ��q 2 � = g 2 ��q 2 �<br />
[1�G �q 2 �] 2 ≃ �g 2 �q 2 �<br />
q 2 �M 2<br />
Taylor efective charge:<br />
2 2 2 2 2<br />
�r�q� = gT ��q � F �q � = gT ���q 2 2<br />
2<br />
� [1�G �q �]<br />
IR efective charge!!<br />
F 2 �q 2 � ≃ �g<br />
2 2<br />
T �q �<br />
q 2 �M 2
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (V)<br />
Next-to-leading asymptotic approximation:<br />
Zero-momentum Taylor-scheme efective charge<br />
A. Aguilar, D. Binosi, J. Papavassiliou, J.R-Q; PRD80(2009)085018<br />
QED-like PT efective charge:<br />
�d �q� = g 2 � ��q 2 � = g 2 ��q 2 �<br />
[1�G �q 2 �] 2 ≃ �g 2 �q 2 �<br />
q 2 �M 2<br />
Taylor efective charge:<br />
2 2 2 2 2<br />
�r�q� = gT ��q � F �q � = gT ���q 2 2<br />
2<br />
� [1�G �q �]<br />
IR efective charge!!<br />
F 2 �q 2 � ≃ �g<br />
2 2<br />
T �q �<br />
q 2 �M 2
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (V)<br />
Next-to-leading asymptotic approximation:<br />
Zero-momentum Taylor-scheme efective charge<br />
A. Aguilar, D. Binosi, J. Papavassiliou, J.R-Q; PRD80(2009)085018<br />
QED-like PT efective charge:<br />
�d �q� = g 2 � ��q 2 � = g 2 ��q 2 �<br />
[1�G �q 2 �] 2 ≃ �g 2 �q 2 �<br />
q 2 �M 2<br />
Taylor efective charge:<br />
2 2 2 2 2<br />
�r�q� = gT ��q � F �q � = gT ���q 2 2<br />
2<br />
� [1�G �q �]<br />
�≃1<br />
IR efective charge!!<br />
F 2 �q 2 � ≃ �g<br />
2 2<br />
T �q �<br />
q 2 �M 2
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (V)<br />
Next-to-leading asymptotic approximation:<br />
Zero-momentum Taylor-scheme efective charge<br />
A. Aguilar, D. Binosi, J. Papavassiliou, J.R-Q; PRD80(2009)085018<br />
QED-like PT efective charge:<br />
�d �q� = g 2 � ��q 2 � = g 2 ��q 2 �<br />
[1�G �q 2 �] 2 ≃ �g 2 �q 2 �<br />
q 2 �M 2<br />
Taylor efective charge:<br />
2 2<br />
2 2 2 2 2<br />
�r�q� = gT ��q � F �q � = gT ���q 2 �g T �q �<br />
� ≃<br />
q 2 �M 2<br />
IR efective charge!!
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (V)<br />
Next-to-leading asymptotic approximation:<br />
Zero-momentum Taylor-scheme efective charge<br />
A. Aguilar, D. Binosi, J. Papavassiliou, J.R-Q; PRD80(2009)085018<br />
�� PT �q 2 � = �g 2 �q 2 �<br />
4� ≃ �� T �q 2 � = �g<br />
2 2<br />
T �q �<br />
4�
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (V)<br />
Next-to-leading asymptotic approximation:<br />
Zero-momentum Taylor-scheme efective charge<br />
A. Aguilar, D. Binosi, J. Papavassiliou, J.R-Q; PRD80(2009)085018<br />
�� PT �q 2 � = �g 2 �q 2 �<br />
4� ≃ �� T �q 2 � = �g<br />
2 2<br />
T �q �<br />
4�
<strong>The</strong> <strong>Ghost</strong>-<strong>propagator</strong> <strong>DSE</strong><br />
solutions (V)<br />
Next-to-leading asymptotic approximation:<br />
Zero-momentum Taylor-scheme efective charge<br />
A. Aguilar, D. Binosi, J. Papavassiliou, J.R-Q; PRD80(2009)085018<br />
�� PT �0� = �g 2 �0�<br />
4� = �� T �0� = �g<br />
2<br />
T �0�<br />
4�<br />
F �0� [1�G �0�]=1
Lattice (recent) results (I)<br />
Gluon <strong>propagator</strong>:<br />
� G =1<br />
(massive solution)<br />
I.L. Bogolubsky, E.M. Ilgenfritz,M. Mulluer-Preussker, A. Sternbeck; arXiv:0901.0736[hep-lat]
Lattice (recent) results (II)<br />
Gluon <strong>propagator</strong>:<br />
� G =1<br />
(massive solution)<br />
O. Oliveira, P. Bicudo ; arXiv:1002.4151[hep-lat]
Lattice (recent) results (III)<br />
Gluon <strong>propagator</strong>:<br />
� G =1<br />
(massive solution)<br />
A. Cuchieri and T. Mendes ; PoS LAT2007 (2007) 297
Lattice (recent) results (IV)<br />
<strong>Ghost</strong> dressing<br />
function:<br />
� F =0<br />
(solution type II,<br />
called also decoupling)<br />
I.L. Bogolubsky, E.M. Ilgenfritz,M. Mulluer-Preussker, A. Sternbeck; arXiv:0901.0736[hep-lat]
Lattice (recent) results (IV)<br />
<strong>Ghost</strong> dressing<br />
function:<br />
� F =0<br />
(solution type II,<br />
called also decoupling)<br />
I.L. Bogolubsky, E.M. Ilgenfritz,M. Mulluer-Preussker, A. Sternbeck; arXiv:0901.0736[hep-lat]
Lattice (recent) results (V)<br />
A few words about Gribov ambiguity
Lattice (recent) results (V)<br />
A few words about Gribov ambiguity<br />
I.L. Bogolubsky, E.M. Ilgenfritz,M. Mulluer-Preussker, A. Sternbeck; arXiv:0901.0736[hep-lat]
Lattice (recent) results (VI)<br />
A few words about Gribov ambiguity<br />
I.L. Bogolubsky, E.M. Ilgenfritz,M. Mulluer-Preussker, A. Sternbeck; arXiv:0901.0736[hep-lat]
Lattice (recent) results (VII)<br />
A few words about Gribov ambiguity<br />
Best copy<br />
vs.<br />
First copy<br />
V.G. Bornyakov, V.K. Mitrjushkin, M. Muller-Preussker; PRD81(2010)054503
Lattice (recent) results (VII)<br />
A few words about Gribov ambiguity<br />
Best copy<br />
vs.<br />
First copy<br />
V.G. Bornyakov, V.K. Mitrjushkin, M. Muller-Preussker; PRD81(2010)054503
Lattice (recent) results (VII)<br />
A few words about Gribov ambiguity<br />
Best copy<br />
vs.<br />
First copy<br />
V.G. Bornyakov, V.K. Mitrjushkin, M. Muller-Preussker; PRD81(2010)054503
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (I)<br />
●In the BFM-PT scheme:<br />
(i) Gluon SDE:<br />
(ii) <strong>Ghost</strong> SDE:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (II)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010<br />
➔ A massive gluon <strong>propagator</strong> is obtained<br />
( �G =1)<br />
➔ A fnite ghost dressing function at zero<br />
momentum is also obtained ( )<br />
� F =0
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (II)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010<br />
➔ A massive gluon <strong>propagator</strong> is obtained<br />
( �G =1)<br />
➔ A fnite ghost dressing function at zero<br />
momentum is also obtained ( )<br />
� F =0
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (II)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010<br />
➔ A massive gluon <strong>propagator</strong> is obtained<br />
( �G =1)<br />
➔ A fnite ghost dressing function at zero<br />
momentum is also obtained ( )<br />
� F =0
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (III)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou; PRD78(2008)025010<br />
J. Rodríguez-Quintero, PRD82(2010)054007
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (III)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou; PRD78(2008)025010<br />
J. Rodríguez-Quintero, PRD82(2010)054007
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (III)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou; PRD78(2008)025010<br />
J. Rodríguez-Quintero, PRD82(2010)054007
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (III)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou; PRD78(2008)025010<br />
J. Rodríguez-Quintero, PRD82(2010)054007
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (III)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou; PRD78(2008)025010<br />
J. Rodríguez-Quintero, PRD82(2010)054007
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (III)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou; PRD78(2008)025010<br />
J. Rodríguez-Quintero, PRD82(2010)054007
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (III)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou; PRD78(2008)025010<br />
J. Rodríguez-Quintero, PRD82(2010)054007
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (III)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou; PRD78(2008)025010<br />
J. Rodríguez-Quintero, PRD82(2010)054007<br />
<strong>The</strong> BFM-PT ghost solutions are very well described by the<br />
asymptotic formula!!!
Part III: <strong>The</strong> scaling strikes back<br />
<strong>The</strong> Scaling
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (IV)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010<br />
Critical value
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (IV)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (IV)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (IV)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (IV)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (IV)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (IV)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (IV)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (IV)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (IV)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (IV)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (IV)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (IV)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010
<strong>Ghost</strong> and gluon coupled <strong>DSE</strong>'s<br />
system (IV)<br />
●In the BFM-PT scheme:<br />
Critical exponent:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010<br />
��10 GeV �=0.0854 �6�
A phase transition between <strong>DSE</strong><br />
solutions? (I)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010
A phase transition between <strong>DSE</strong><br />
solutions? (I)<br />
●In the BFM-PT scheme:<br />
� F =0<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010
A phase transition between <strong>DSE</strong><br />
solutions? (I)<br />
●In the BFM-PT scheme:<br />
� F =0<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010<br />
Critical value<br />
� F ≠0
A phase transition between <strong>DSE</strong><br />
solutions? (I)<br />
●In the BFM-PT scheme:<br />
If � G =1 F �q 2 � ~ 1<br />
� F =0<br />
�q 2<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010<br />
Critical value<br />
� F ≠0
A phase transition between <strong>DSE</strong><br />
solutions? (I)<br />
●In the BFM-PT scheme:<br />
If � G =1 F �q 2 � ~ 1<br />
� F =0<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010<br />
�q 2 � G � 1<br />
Critical value<br />
� F ≠0
A phase transition between <strong>DSE</strong><br />
solutions? (I)<br />
●In the BFM-PT scheme:<br />
If � G =1 F �q 2 � ~ 1<br />
� F =0<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010<br />
�q 2 � G � 1<br />
Critical value<br />
� F ≠0
A phase transition between <strong>DSE</strong><br />
solutions? (II)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010
A phase transition between <strong>DSE</strong><br />
solutions? (II)<br />
●In the BFM-PT scheme:<br />
1<br />
F R �0�<br />
≠ 0<br />
IR ghost non-dominance<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010<br />
IR ghost dominance<br />
1<br />
F R �0�<br />
� 0
A phase transition between <strong>DSE</strong><br />
solutions? (II)<br />
●In the BFM-PT scheme:<br />
A.C.Aguilar, D.Binosi, J.Papavassiliou;<br />
PRD78(2008)025010<br />
Order parameter?<br />
1<br />
F R �0�<br />
≠ 0<br />
IR ghost non-dominance<br />
IR ghost dominance<br />
1<br />
F R �0�<br />
� 0
Conclusions:<br />
●<strong>The</strong> ghost <strong>propagator</strong> <strong>DSE</strong> allows for solutions observing<br />
two types of IR behaviors:<br />
➔ I: Divergent ghost dressing function and a fnite ghost-gluon<br />
coupling at zero momentum (“scaling” or “conformal”)<br />
➔ II: Finite ghost dressing function and massive gluon <strong>propagator</strong>,<br />
with a vanishing ghost-gluon coupling at zero-momentum<br />
(“decoupling”).<br />
●(Yang-Mills) Lattice QCD clearly favors the ”decoupling”<br />
●In the BFM-PT scheme, the <strong>DSE</strong> coupled system for ghost<br />
and gluon <strong>propagator</strong>s, massive gluon and not-enhanced<br />
ghost (“decoupling”) solutions emerge.<br />
●A low-momentum asymptotic formula for the ghost<br />
dressing function perfectly agrees with numerical results.
●<br />
Conclusions:<br />
➔ I: Divergent ghost dressing function and a fnite ghost-gluon<br />
coupling at zero momentum (“scaling” or “conformal”)<br />
➔ II: Finite ghost dressing function and massive gluon <strong>propagator</strong>,<br />
with a vanishing ghost-gluon coupling at zero-momentum<br />
(“decoupling”).<br />
●(Yang-Mills) Lattice QCD clearly favors the ”decoupling”<br />
●In the BFM-PT scheme, the <strong>DSE</strong> coupled system for ghost<br />
and gluon <strong>propagator</strong>s, massive gluon and not-enhanced<br />
ghost (“decoupling”) solutions emerge.<br />
●A low-momentum asymptotic formula for the ghost<br />
dressing function perfectly agrees with numerical results.<br />
●A sort of phase transition between both types of solutions<br />
appears to take place.
Conclusions:<br />
●<br />
●(Yang-Mills) Lattice QCD clearly favors the ”decoupling”<br />
●In the BFM-PT scheme, the <strong>DSE</strong> coupled system for ghost<br />
and gluon <strong>propagator</strong>s, massive gluon and not-enhanced<br />
ghost (“decoupling”) solutions emerge.<br />
●A low-momentum asymptotic formula for the ghost<br />
dressing function perfectly agrees with numerical results.<br />
●A sort of phase transition between both types of solutions<br />
appears to take place.<br />
●<strong>The</strong> control parameter “dialing” the transition is the<br />
Taylor-scheme coupling constant.
Conclusions:<br />
●A low-momentum asymptotic formula for the ghost<br />
dressing function perfectly agrees with numerical results.<br />
●A sort of phase transition between both types of solutions<br />
appears to take place.<br />
●<strong>The</strong> control parameter “dialing” the transition is the<br />
Taylor-scheme coupling constant.<br />
●<strong>The</strong> role of the order parameter is played by the inverse<br />
of the ghost dressing, which vanishes at the critical point.<br />
●Is this order parameter related to some condensate?<br />
Kugo-Ojima and Gribov-Zwanziger confnement scenarios, ghost<br />
dominance... ???????
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