-
1
-
-
8744222241
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.22.981
-
J.J. Sakurai, Phys. Rev. Lett. 22, 981 (1969). PRLTAO 0031-9007 10.1103/PhysRevLett.22.981
-
(1969)
Phys. Rev. Lett.
, vol.22
, pp. 981
-
-
Sakurai, J.J.1
-
3
-
-
0001393702
-
-
PHRVAO 0031-899X 10.1103/PhysRev.124.953
-
M. Gell-Mann and F. Zachariasen, Phys. Rev. 124, 953 (1961). PHRVAO 0031-899X 10.1103/PhysRev.124.953
-
(1961)
Phys. Rev.
, vol.124
, pp. 953
-
-
Gell-Mann, M.1
Zachariasen, F.2
-
4
-
-
36049054596
-
-
PHRVAO 0031-899X 10.1103/PhysRev.157.1376
-
N.M. Kroll, T.D. Lee, and B. Zumino, Phys. Rev. 157, 1376 (1967). PHRVAO 0031-899X 10.1103/PhysRev.157.1376
-
(1967)
Phys. Rev.
, vol.157
, pp. 1376
-
-
Kroll, N.M.1
Lee, T.D.2
Zumino, B.3
-
5
-
-
0001313970
-
-
PHRVAO 0031-899X 10.1103/PhysRev.106.1366
-
Y. Nambu, Phys. Rev. 106, 1366 (1957). PHRVAO 0031-899X 10.1103/PhysRev.106.1366
-
(1957)
Phys. Rev.
, vol.106
, pp. 1366
-
-
Nambu, Y.1
-
6
-
-
84989002378
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.2.365
-
W.R. Frazer and J. Fulco, Phys. Rev. Lett. 2, 365 (1959). PRLTAO 0031-9007 10.1103/PhysRevLett.2.365
-
(1959)
Phys. Rev. Lett.
, vol.2
, pp. 365
-
-
Frazer, W.R.1
Fulco, J.2
-
7
-
-
4243428304
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.18.2484
-
J. Orear, Phys. Rev. D PRVDAQ 0556-2821 18, 2484 (1978). 10.1103/PhysRevD.18.2484
-
(1978)
Phys. Rev. D
, vol.18
, pp. 2484
-
-
Orear, J.1
-
8
-
-
0038236460
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.67.094004
-
R. Petronzio, S. Simula, and G. Ricco, Phys. Rev. D 67, 094004 (2003); PRVDAQ 0556-2821 10.1103/PhysRevD.67.094004
-
(2003)
Phys. Rev. D
, vol.67
, pp. 094004
-
-
Petronzio, R.1
Simula, S.2
Ricco, G.3
-
10
-
-
0000067899
-
-
PYLBAJ 0370-2693 10.1016/0370-2693(73)90266-9
-
F. Iachello, A.D. Jackson, and A. Lande, Phys. Lett. 43B, 191 (1973); PYLBAJ 0370-2693 10.1016/0370-2693(73)90266-9
-
(1973)
Phys. Lett.
, vol.43
, pp. 191
-
-
Iachello, F.1
Jackson, A.D.2
Lande, A.3
-
11
-
-
4043101159
-
-
PRVCAN 0556-2813 10.1103/PhysRevC.69.068201
-
R. Bijker and F. Iachello, Phys. Rev. C 69, 068201 (2004). PRVCAN 0556-2813 10.1103/PhysRevC.69.068201
-
(2004)
Phys. Rev. C
, vol.69
, pp. 068201
-
-
Bijker, R.1
Iachello, F.2
-
12
-
-
0000494033
-
-
NUPABL 0375-9474 10.1016/0375-9474(86)90112-0
-
G.E. Brown, M. Rho, and W. Weise, Nucl. Phys. NUPABL 0375-9474 A454, 669 (1986). 10.1016/0375-9474(86)90112-0
-
(1986)
Nucl. Phys.
, vol.454
, pp. 669
-
-
Brown, G.E.1
Rho, M.2
Weise, W.3
-
13
-
-
34948847036
-
-
JHEPFG 1029-8479 10.1088/1126-6708/2007/09/063
-
D.K. Hong, M. Rho, H.U. Yee, and P. Yi, J. High Energy Phys. JHEPFG 1029-8479 09 (2007) 063. 10.1088/1126-6708/2007/09/063
-
J. High Energy Phys.
, vol.2007
, Issue.9
, pp. 063
-
-
Hong, D.K.1
Rho, M.2
Yee, H.U.3
Yi, P.4
-
14
-
-
22144432992
-
-
PTPKAV 0033-068X 10.1143/PTP.113.843
-
T. Sakai and S. Sugimoto, Prog. Theor. Phys. 113, 843 (2005); PTPKAV 0033-068X 10.1143/PTP.113.843
-
(2005)
Prog. Theor. Phys.
, vol.113
, pp. 843
-
-
Sakai, T.1
Sugimoto, S.2
-
15
-
-
32044442269
-
-
PTPKAV 0033-068X 10.1143/PTP.114.1083
-
T. Sakai S. Sugimoto Prog. Theor. Phys. 114, 1083 (2005). PTPKAV 0033-068X 10.1143/PTP.114.1083
-
(2005)
Prog. Theor. Phys.
, vol.114
, pp. 1083
-
-
Sakai, T.1
Sugimoto, S.2
-
17
-
-
34250837962
-
-
PYLBAJ 0370-2693 10.1016/j.physletb.2007.05.044
-
H.R. Grigoryan and A.V. Radyushkin, Phys. Lett. B 650, 421 (2007); PYLBAJ 0370-2693 10.1016/j.physletb.2007.05.044
-
(2007)
Phys. Lett. B
, vol.650
, pp. 421
-
-
Grigoryan, H.R.1
Radyushkin, A.V.2
-
20
-
-
34748925398
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.76.061901
-
D.K. Hong, M. Rho, H.U. Yee, and P. Yi, Phys. Rev. D 76, 061901 (2007). PRVDAQ 0556-2821 10.1103/PhysRevD.76.061901
-
(2007)
Phys. Rev. D
, vol.76
, pp. 061901
-
-
Hong, D.K.1
Rho, M.2
Yee, H.U.3
Yi, P.4
-
21
-
-
38849182786
-
-
See Ref. for a detailed mass spectrum. References discuss bottom-up phenomenological models.
-
See Ref. for a detailed mass spectrum. References discuss bottom-up phenomenological models.
-
-
-
-
22
-
-
38849143903
-
-
In the Skyrme model where only the pion field is present, surrounded by the vector-meson (ρ, ω, etc.) cloud, the extended object, i.e., the skyrmion, plays a crucial role, representing the core in the form factor and cannot be transformed away as is done in the SS model. This is one more indication-in addition to what was argued in -that our instanton baryon in hQCD is basically different from the standard skyrmion made up of the pion field only.
-
In the Skyrme model where only the pion field is present, surrounded by the vector-meson (ρ, ω, etc.) cloud, the extended object, i.e., the skyrmion, plays a crucial role, representing the core in the form factor and cannot be transformed away as is done in the SS model. This is one more indication-in addition to what was argued in -that our instanton baryon in hQCD is basically different from the standard skyrmion made up of the pion field only.
-
-
-
-
23
-
-
38849187224
-
-
This procedure does not involve mesonic loop graphs that bring in higher order corrections in the 1/Nc expansion. It naturally comes in a simple bookkeeping of symmetry for the spin-isospin operators figuring in the Gamow-Teller operator and the isovector magnetic moment operator in electroweak processes as explained in.
-
This procedure does not involve mesonic loop graphs that bring in higher order corrections in the 1/Nc expansion. It naturally comes in a simple bookkeeping of symmetry for the spin-isospin operators figuring in the Gamow-Teller operator and the isovector magnetic moment operator in electroweak processes as explained in.
-
-
-
-
24
-
-
84951609709
-
-
ZPAHEX 0939-7922
-
G. Holzwarth, Z. Phys. A ZPAHEX 0939-7922 356, 339 (1996).
-
(1996)
Z. Phys. a
, vol.356
, pp. 339
-
-
Holzwarth, G.1
-
27
-
-
38849104407
-
-
note
-
It is perhaps worth stressing that all the parameters of the theory to be used to describe baryons are completely fixed in the meson sector. This should be contrasted to what is done in the standard approach to skyrmion physics where the parameters of the chiral Lagrangian figuring in the baryon sector are required to be drastically different from those of the meson sector. For instance, with the Skyrme Lagrangian which has three parameters, Fπ, mπ, and e, if one fixes mπ to the physical value, then the effective pion decay constant needed for the nucleon and the Δ comes out to be much smaller, say 50%, than the experimental value. On the other hand, if one were to use the Skyrme model for describing nuclei-which is a legitimate thing to do-the effective pion mass required comes out to be ∼2 times the physical value in order to have a sensible nuclear structure. Thus the basic strategy of building a large Nc meson Lagrangian to apply to the baryon sector fails badly with chiral Lagrangians without vector-meson degrees of freedom.
-
-
-
-
28
-
-
2142653509
-
-
NUPABL 0375-9474 10.1016/j.nuclphysa.2004.03.002
-
M. Harada and C. Sasaki, Nucl. Phys. NUPABL 0375-9474 A736, 300 (2004). 10.1016/j.nuclphysa.2004.03.002
-
(2004)
Nucl. Phys.
, vol.736
, pp. 300
-
-
Harada, M.1
Sasaki, C.2
-
34
-
-
0037780975
-
-
PRPLCM 0370-1573 10.1016/S0370-1573(03)00139-X
-
M. Harada and K. Yamawaki, Phys. Rep. 381, 1 (2003). PRPLCM 0370-1573 10.1016/S0370-1573(03)00139-X
-
(2003)
Phys. Rep.
, vol.381
, pp. 1
-
-
Harada, M.1
Yamawaki, K.2
-
35
-
-
33750001676
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.74.076004
-
M. Harada, S. Matsuzaki, and K. Yamawaki, Phys. Rev. D 74, 076004 (2006). PRVDAQ 0556-2821 10.1103/PhysRevD.74.076004
-
(2006)
Phys. Rev. D
, vol.74
, pp. 076004
-
-
Harada, M.1
Matsuzaki, S.2
Yamawaki, K.3
-
36
-
-
38849124246
-
-
arXiv:hep-ph/0703264.
-
M. Rho, arXiv:hep-ph/0703264.
-
-
-
Rho, M.1
-
37
-
-
2342440134
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.69.065020
-
D.T. Son and M.A. Stephanov, Phys. Rev. D 69, 065020 (2004). PRVDAQ 0556-2821 10.1103/PhysRevD.69.065020
-
(2004)
Phys. Rev. D
, vol.69
, pp. 065020
-
-
Son, D.T.1
Stephanov, M.A.2
-
38
-
-
37649030726
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.87.152001
-
M. Harada and K. Yamawaki, Phys. Rev. Lett. 87, 152001 (2001). PRLTAO 0031-9007 10.1103/PhysRevLett.87.152001
-
(2001)
Phys. Rev. Lett.
, vol.87
, pp. 152001
-
-
Harada, M.1
Yamawaki, K.2
-
39
-
-
33947692783
-
-
JHEPFG 1029-8479 10.1088/1126-6708/2007/01/072
-
N. Horigome and Y. Tanii, J. High Energy Phys. JHEPFG 1029-8479 01 (2007) 072; 10.1088/1126-6708/2007/01/072
-
J. High Energy Phys.
, vol.2007
, Issue.1
, pp. 072
-
-
Horigome, N.1
Tanii, Y.2
-
41
-
-
33947698902
-
-
JHEPFG 1029-8479 10.1088/1126-6708/2007/02/016
-
S. Kobayashi, D. Mateos, S. Matsuura, R.C. Myers, and R.M. Thomson, J. High Energy Phys. JHEPFG 1029-8479 02 (2007) 016. 10.1088/1126-6708/2007/02/016
-
J. High Energy Phys.
, vol.2007
, Issue.2
, pp. 016
-
-
Kobayashi, S.1
Mateos, D.2
Matsuura, S.3
Myers, R.C.4
Thomson, R.M.5
-
42
-
-
18744436199
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.84.1398
-
M.K. Jones (Jefferson Lab Hall A Collaboration), Phys. Rev. Lett. 84, 1398 (2000). PRLTAO 0031-9007 10.1103/PhysRevLett.84.1398
-
(2000)
Phys. Rev. Lett.
, vol.84
, pp. 1398
-
-
Jones, M.K.1
-
43
-
-
33750676797
-
-
PRVDAQ 0556-2821 10.1103/PhysRevD.49.5671
-
R.C. Walker, Phys. Rev. D 49, 5671 (1994). PRVDAQ 0556-2821 10.1103/PhysRevD.49.5671
-
(1994)
Phys. Rev. D
, vol.49
, pp. 5671
-
-
Walker, R.C.1
-
45
-
-
26944432989
-
-
PRLTAO 0031-9007 10.1103/PhysRevLett.94.201601
-
G.F. de Teramond and S.J. Brodsky, Phys. Rev. Lett. 94, 201601 (2005); PRLTAO 0031-9007 10.1103/PhysRevLett.94.201601
-
(2005)
Phys. Rev. Lett.
, vol.94
, pp. 201601
-
-
De Teramond, G.F.1
Brodsky, S.J.2
-
46
-
-
33847256929
-
-
PYLBAJ 0370-2693 10.1016/j.physletb.2007.01.030
-
D.K. Hong, T. Inami, and H.U. Yee, Phys. Lett. B 646, 165 (2007); PYLBAJ 0370-2693 10.1016/j.physletb.2007.01.030
-
(2007)
Phys. Lett. B
, vol.646
, pp. 165
-
-
Hong, D.K.1
Inami, T.2
Yee, H.U.3
-
47
-
-
36849078954
-
-
JHEPFG 1029-8479 10.1088/1126-6708/2007/11/036
-
D.K. Hong, H.C. Kim, S. Siwach, and H.U. Yee, J. High Energy Phys. JHEPFG 1029-8479 11 (2007) 036. 10.1088/1126-6708/2007/11/036
-
J. High Energy Phys.
, vol.2007
, Issue.11
, pp. 036
-
-
Hong, D.K.1
Kim, H.C.2
Siwach, S.3
Yee, H.U.4
-
48
-
-
25844491783
-
-
PYLBAJ 0370-2693 10.1016/j.physletb.2005.08.097
-
R.A. Battye, S. Krusch, and P.M. Sutcliffe, Phys. Lett. B 626, 120 (2005). PYLBAJ 0370-2693 10.1016/j.physletb.2005.08.097
-
(2005)
Phys. Lett. B
, vol.626
, pp. 120
-
-
Battye, R.A.1
Krusch, S.2
Sutcliffe, P.M.3
|