-
5
-
-
0037122824
-
-
C.A. Scrucca, M. Serone, L. Silvestrini, and F. Zwirner, Phys. Lett. B 525, 169 (2002).
-
(2002)
Phys. Lett. B
, vol.525
, pp. 169
-
-
Scrucca, C.A.1
Serone, M.2
Silvestrini, L.3
Zwirner, F.4
-
6
-
-
0037101402
-
-
R. Barbieri, R. Contino, P. Creminelli, R. Rattazzi, and C.A. Scrucca, Phys. Rev. D 66, 024025 (2002).
-
(2002)
Phys. Rev. D
, vol.66
, pp. 24025
-
-
Barbieri, R.1
Contino, R.2
Creminelli, P.3
Rattazzi, R.4
Scrucca, C.A.5
-
7
-
-
0035797172
-
-
N. Arkani-Hamed, L.J. Hall, Y. Nomura, D.R. Smith, and N. Weiner, Nucl. Phys. B605, 81 (2001).
-
(2001)
Nucl. Phys.
, vol.B605
, pp. 81
-
-
Arkani-Hamed, N.1
Hall, L.J.2
Nomura, Y.3
Smith, D.R.4
Weiner, N.5
-
12
-
-
0001310354
-
-
R. Barbieri, S. Ferrara, D.V. Nanopoulos, and K.S. Stelle, Phys. Lett. 113B, 219 (1982).
-
(1982)
Phys. Lett.
, vol.113B
, pp. 219
-
-
Barbieri, R.1
Ferrara, S.2
Nanopoulos, D.V.3
Stelle, K.S.4
-
13
-
-
0001539969
-
-
S. Ferrara, L. Girardello, T. Kugo, and A. Van Proeyen, Nucl. Phys. B223, 191 (1983).
-
(1983)
Nucl. Phys.
, vol.B223
, pp. 191
-
-
Ferrara, S.1
Girardello, L.2
Kugo, T.3
Van Proeyen, A.4
-
15
-
-
0033548816
-
-
I. Antoniadis, S. Dimopoulos, A. Pomarol, and M. Quiros, Nucl. Phys. B544, 503 (1999).
-
(1999)
Nucl. Phys.
, vol.B544
, pp. 503
-
-
Antoniadis, I.1
Dimopoulos, S.2
Pomarol, A.3
Quiros, M.4
-
18
-
-
85038273467
-
-
Proceedings of the APS/DPF/DPB Summer Study on the Future of Particle Physics (Snowmass, 2001), edited by R. Davidson and C. Quigg, hep-ph/0112001
-
M. Chertok, G.D. Kribs, Y. Nomura, W. Orejudos, B. Schumm, and S. Su, in Proceedings of the APS/DPF/DPB Summer Study on the Future of Particle Physics (Snowmass, 2001), edited by R. Davidson and C. Quigg, hep-ph/0112001.
-
-
-
Chertok, M.1
Kribs, G.D.2
Nomura, Y.3
Orejudos, W.4
Schumm, B.5
Su, S.6
-
20
-
-
85038273950
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A factor of 2 is included to account for the coupling of the nonzero KK modes, (Formula presented) times stronger than for the zero mode.
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A factor of 2 is included to account for the coupling of the nonzero KK modes, (Formula presented) times stronger than for the zero mode.
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21
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85038330674
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The lightest top squark now comes in two degenerate chiralities.
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The lightest top squark now comes in two degenerate chiralities.
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22
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85038333108
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Here we are working on the interval (Formula presented)
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Here we are working on the interval (Formula presented)
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23
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85038324748
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Using the formulation in terms of 4D (Formula presented) superfields 19 one privileges only one of the two local supersymmetries, here (Formula presented) This explains the apparent asymmetry between (Formula presented) and (Formula presented)
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Using the formulation in terms of 4D (Formula presented) superfields 19 one privileges only one of the two local supersymmetries, here (Formula presented) This explains the apparent asymmetry between (Formula presented) and (Formula presented)
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24
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85038325347
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Or on (Formula presented) and (Formula presented)
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Or on (Formula presented) and (Formula presented)
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