Splitting split supersymmetry

被引:21
作者
Cheung, K [1 ]
Chiang, CW
机构
[1] Natl Tsing Hua Univ, Dept Phys, Hsinchu, Taiwan
[2] Natl Tsing Hua Univ, NCTS, Hsinchu, Taiwan
[3] Natl Cent Univ, Dept Phys, Chungli 320, Taiwan
[4] Acad Sinica, Inst Phys, Taipei 115, Taiwan
来源
PHYSICAL REVIEW D | 2005年 / 71卷 / 09期
关键词
D O I
10.1103/PhysRevD.71.095003
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In split supersymmetry, the supersymmetric scalar particles are all very heavy, at least at the order of 10(9) GeV, but the gauginos, Higgsinos, and one of the neutral Higgs bosons remain below a TeV. Here we further split the split supersymmetry by taking the Higgsino mass parameter mu to be very large. In this case, the mu problem is avoided and we keep the wino as a dark matter candidate. A crude gauge-coupling unification is still preserved. Dark matter signals and collider phenomenology are discussed in this mu-split SUSY scenario. The most interesting dark matter signal is the annihilation into monochromatic photons. In colliders, chargino-pair and the associated chargino-neutralino production cross sections have a certain ratio due to gauge couplings.
引用
收藏
页码:1 / 9
页数:9
相关论文
共 44 条
[1]   Search for the standard model Higgs boson at LEP [J].
Abbaneo, D ;
Abbiendi, G ;
Barate, R ;
Heister, A ;
Schael, S ;
Barate, R ;
Bruneliere, R ;
De Bonis, I ;
Decamp, D ;
Goy, C ;
Jezequel, S ;
Lees, JP ;
Martin, F ;
Merle, E ;
Minard, MN ;
Pietrzyk, B ;
Trocme, B ;
Boix, G ;
Bravo, S ;
Casado, MP ;
Chmeissani, M ;
Crespo, JM ;
Fernandez, E ;
Fernandez-Bosman, M ;
Garrido, L ;
Grauges, E ;
Lopez, J ;
Martinez, M ;
Merino, G ;
Miquel, R ;
Mir, LM ;
Pacheco, A ;
Paneque, D ;
Ruiz, H ;
Colaleo, A ;
Creanza, D ;
De Filippis, N ;
de Palma, M ;
Iaselli, G ;
Maggi, G ;
Maggi, M ;
Nuzzo, S ;
Ranieri, A ;
Raso, G ;
Ruggieri, F ;
Selvaggi, G ;
Silvestris, L ;
Tempesta, P ;
Tricomi, A ;
Zito, G .
PHYSICS LETTERS B, 2003, 565 (1-4) :61-75
[2]   The Alpha Magnetic Spectrometer (AMS) on the International Space Station:: Part I -: results from the test flight on the space shuttle [J].
Aguilar, M ;
Alcaraz, J ;
Allaby, J ;
Alpat, B ;
Ambrosi, G ;
Anderhub, H ;
Ao, L ;
Arefiev, A ;
Azzarello, P ;
Babucci, E ;
Baldini, L ;
Basile, M ;
Barancourt, D ;
Barao, F ;
Barbier, G ;
Barreira, G ;
Battiston, R ;
Becker, R ;
Becker, U ;
Bellagamba, L ;
Béné, P ;
Berdugo, J ;
Berges, P ;
Bertucci, B ;
Biland, A ;
Bizzaglia, S ;
Blasko, S ;
Boella, G ;
Boschini, M ;
Bourquin, M ;
Brocco, L ;
Bruni, G ;
Buénerd, M ;
Burger, JD ;
Burger, WJ ;
Cai, XD ;
Camps, C ;
Cannarsa, P ;
Capell, M ;
Casadei, D ;
Casaus, J ;
Castellini, G ;
Cecchi, C ;
Chang, YH ;
Chen, HF ;
Chen, HS ;
Chen, ZG ;
Chernoplekov, NA ;
Chiueh, TH ;
Cho, K .
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 2002, 366 (06) :331-405
[3]  
[Anonymous], 2003, PHYS REPT
[4]   Aspects of split supersymmetry [J].
Arkani-Hamed, N ;
Dimopoulos, S ;
Giudice, GF ;
Romanino, A .
NUCLEAR PHYSICS B, 2005, 709 (1-2) :3-46
[5]  
ARKANIHAMED N, HEPTH0405159
[6]  
BABU KS, HEPPH0501079
[7]   Heavy gluino as the lightest supersymmetric particle [J].
Baer, H ;
Cheung, K ;
Gunion, JF .
PHYSICAL REVIEW D, 1999, 59 (07)
[8]   Axion models with high-scale supersymmetry breaking [J].
Barger, V ;
Chiang, CW ;
Jiang, J ;
Li, TJ .
NUCLEAR PHYSICS B, 2005, 705 (1-2) :71-91
[9]   First-year Wilkinson Microwave Anisotropy Probe (WMAP) observations:: Preliminary maps and basic results [J].
Bennett, CL ;
Halpern, M ;
Hinshaw, G ;
Jarosik, N ;
Kogut, A ;
Limon, M ;
Meyer, SS ;
Page, L ;
Spergel, DN ;
Tucker, GS ;
Wollack, E ;
Wright, EL ;
Barnes, C ;
Greason, MR ;
Hill, RS ;
Komatsu, E ;
Nolta, MR ;
Odegard, N ;
Peiris, HV ;
Verde, L ;
Weiland, JL .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2003, 148 (01) :1-27
[10]   Full one-loop calculation of neutralino annihilation into two photons [J].
Bergstrom, L ;
Ullio, P .
NUCLEAR PHYSICS B, 1997, 504 (1-2) :27-44