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2011 QCD and High Energy Interactions - Rencontres de Moriond ...

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√ 2<br />

3 MKK<br />

mass<br />

✻<br />

✻<br />

❄<br />

✻<br />

❄<br />

✻<br />

❄<br />

J P<br />

1<br />

2<br />

+ 1<br />

2<br />

− 3<br />

2<br />

+ 3 −<br />

2<br />

mass (GeV)<br />

2 ✻<br />

1.5<br />

1<br />

1<br />

2<br />

+ 1<br />

2<br />

− 3<br />

2<br />

+ 3 −<br />

2<br />

Figure 3: Left si<strong>de</strong> is the baryon spectrum obtained in the mo<strong>de</strong>l, while the right si<strong>de</strong> is the spectrum of the<br />

baryons with I = J taken from particle listings by Particle Data Group. Here I <strong>and</strong> J are the isospin <strong>and</strong> spin,<br />

respectively, <strong>and</strong> <strong>and</strong> P is the parity.<br />

the techniques <strong>de</strong>veloped in the Skyrme mo<strong>de</strong>l to our system, we can analyze various properties<br />

of baryons. The spectrum of the baryon is obtained as in Figure 3. It is interesting to note<br />

that our result suggests that second lightest baryon with J P = 1 +<br />

2 <strong>and</strong> the lightest one with<br />

J P = 1 −<br />

2 are <strong>de</strong>generate. This feature is found in the experiment <strong>and</strong> has been a mystery in<br />

hadron physics for a long time. The results for the charge radii <strong>and</strong> magnetic moments for<br />

nucleons are listed in Table 2.<br />

Table 2: 〈 r 2〉<br />

I=0 , 〈 r 2〉<br />

I=1 <strong>and</strong> 〈 r 2〉<br />

Acknowledgments<br />

are isoscalar, isovector <strong>and</strong> axial mean square radii, respectively. gI=0 <strong>and</strong><br />

A<br />

gI=1 are isoscalar <strong>and</strong> isovector g-factors. gA is the axial coupling.<br />

〈<br />

2<br />

r 〉<br />

〈 I=0<br />

2<br />

r 〉<br />

〈 I=1<br />

2<br />

r 〉<br />

our mo<strong>de</strong>l experiment<br />

(0.74 fm) 2<br />

(0.81 fm) 2<br />

(0.74 fm) 2<br />

(0.94 fm) 2<br />

(0.54 fm) 2<br />

(0.67 fm) 2<br />

A<br />

gI=0 1.7 1.8<br />

gI=1 7.0 9.4<br />

gA 0.73 1.3<br />

We would like to thank the organizers of the <strong>Moriond</strong> workshop for kind invitation <strong>and</strong> hospitality.<br />

We are also grateful to K. Hashimoto, H. Hata, T. Imoto, T. Sakai, <strong>and</strong> S. Yamato<br />

for pleasant collaborations. This work is supported in part by the Grant-in-Aid for Young Scientists<br />

(B), Ministry of Education, Culture, Sports, Science <strong>and</strong> Technology (MEXT), Japan,<br />

JSPS Grant-in-Aid for Creative Scientific Research No. 19GS0219 <strong>and</strong> also by World Premier<br />

International Research Center Initiative (WPI Initiative), MEXT, Japan.<br />

References b<br />

1. T. Sakai, S. Sugimoto, Prog. Theor. Phys. 113, 843-882 (2005).<br />

2. T. Sakai, S. Sugimoto, Prog. Theor. Phys. 114, 1083-1118 (2005).<br />

3. H. Hata, T. Sakai, S. Sugimoto, S. Yamato, Prog. Theor. Phys. 117, 1157 (2007).<br />

4. K. Hashimoto, T. Sakai, S. Sugimoto, Prog. Theor. Phys. 120, 1093-1137 (2008).<br />

5. T. Imoto, T. Sakai, S. Sugimoto, Prog. Theor. Phys. 124, 263-284 (2010).<br />

6. E. Witten, Adv. Theor. Math. Phys. 2, 505 (1998)<br />

b We apologize for not being able to cite all the relevant references. See the references in our papers. 1,2,3,4,5

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