Model independent approach to focus point supersymmetry: from dark matter to collider searches

被引:91
作者
Baer, H [1 ]
Krupovnickas, T
Profumo, S
Ullio, P
机构
[1] Florida State Univ, Dept Phys, Tallahassee, FL 32306 USA
[2] Brookhaven Natl Lab, High Energy Theory Grp, Upton, NY 11973 USA
[3] SISSA, ISAS, I-34013 Trieste, Italy
来源
JOURNAL OF HIGH ENERGY PHYSICS | 2005年 / 10期
关键词
dark matter and double beta decay; Hadron-Hadron scattering; supersymmetry phenomenology;
D O I
10.1088/1126-6708/2005/10/020
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
The focus point region of supersymmetric models is compelling in that it simultaneously features low fine-tuning, provides a decoupling solution to the SUSY flavor and CP problems, suppresses proton decay rates and can accommodate the WMAP measured cold dark matter (DM) relic density through a mixed bino-higgsino dark matter particle. We present the focus point region in terms of a weak scale parameterization, which allows for a relatively model independent compilation of phenomenological constraints and prospects. We present direct and indirect neutralino dark matter detection rates for two different halo density profiles, and show that prospects for direct DM detection and indirect detection via neutrino telescopes such as IceCube and anti-deuteron searches by GAPS are especially promising. We also present LHC reach prospects via gluino and squark cascade decay searches, and also via clean trilepton signatures arising from chargino-neutralino production. Both methods provide a reach out to m(g) similar to 1.7TeV. At a TeV-scale linear e(+)e(-) collider (LC), the maximal reach is attained in the Z(1)Z(2) or Z(1)Z(3) channels. In the DM allowed region of parameter space, a root s = 0.5TeV LC has a reach which is comparable to that of the LHC. However, the reach of a 1TeV LC extends out to m(g) similar to 3.5TeV.
引用
收藏
页码:495 / 532
页数:38
相关论文
共 119 条
[1]   Discovery potential for supersymmetry in CMS [J].
Abdullin, S ;
Antunovic, Z ;
Charles, F ;
Denegri, D ;
Dydak, U ;
Dzelalija, M ;
Genchev, V ;
Graham, D ;
Iashvili, I ;
Kharchilava, A ;
Kinnunen, R ;
Kunori, S ;
Mazumdar, K ;
Racca, C ;
Rurua, L ;
Stepanov, N ;
Womersley, J .
JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS, 2002, 28 (03) :469-594
[2]   Search for SUSY in (leptons plus) jets plus ETmiss final states [J].
Abdullin, S ;
Charles, F .
NUCLEAR PHYSICS B, 1999, 547 (1-2) :60-80
[3]   AN ANTIMATTER SPECTROMETER IN-SPACE [J].
AHLEN, S ;
BALEBANOV, VM ;
BATTISTON, R ;
BECKER, U ;
BURGER, J ;
CAPELL, M ;
CHEN, HF ;
CHEN, HS ;
CHEN, M ;
CHERNOPLEKOV, N ;
CLARE, R ;
DAI, TS ;
DERUJULA, A ;
FISHER, P ;
GALAKTIONOV, Y ;
GOUGAS, A ;
GU, WQ ;
HE, M ;
KOUTSENKO, V ;
LEBEDEV, A ;
LI, TP ;
LU, YS ;
LUCKEY, D ;
MA, Y ;
MCNEIL, R ;
ORAVA, R ;
PREVSNER, A ;
PLYASKINE, V ;
RUBINSTEIN, H ;
SAGDEEV, R ;
SALAMON, M ;
TANG, HW ;
TING, SCC ;
VETLITSKY, I ;
WANG, YF ;
XIA, PC ;
XU, ZZ ;
WEFEL, JP ;
ZHANG, ZP ;
ZHOU, B ;
ZICHICHI, A .
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 1994, 350 (1-2) :351-367
[4]   First results from the cryogenic dark matter search in the Soudan Underground Laboratory [J].
Akerib, DS ;
Alvaro-Dean, J ;
Armel-Funkhouser, MS ;
Attisha, MJ ;
Baudis, L ;
Bauer, DA ;
Beaty, J ;
Brink, PL ;
Bunker, R ;
Burke, SP ;
Cabrera, B ;
Caldwell, DO ;
Callahan, D ;
Castle, JP ;
Chang, CL ;
Choate, R ;
Crisler, MB ;
Cushman, P ;
Dixon, R ;
Dragowsky, MR ;
Driscoll, DD ;
Duong, L ;
Emes, J ;
Ferril, R ;
Filippini, J ;
Gaitskell, RJ ;
Haldeman, M ;
Hale, D ;
Holmgren, D ;
Huber, ME ;
Johnson, B ;
Johnson, W ;
Kamat, S ;
Kozlovsky, M ;
Kula, L ;
Kyre, S ;
Lambin, B ;
Lu, A ;
Mahapatra, R ;
Manalaysay, AG ;
Mandic, V ;
May, J ;
McDonald, R ;
Merkel, B ;
Meunier, P ;
Mirabolfathi, N ;
Morrison, S ;
Nelson, H ;
Nelson, R ;
Novak, L .
PHYSICAL REVIEW LETTERS, 2004, 93 (21)
[5]  
ALLANACH B, HEPPH0207314, P9
[6]   Theoretical uncertainties in sparticle mass predictions from computational tools [J].
Allanach, BC ;
Kraml, S ;
Porod, W .
JOURNAL OF HIGH ENERGY PHYSICS, 2003, (03) :353-373
[7]  
Allanach BC, 2000, J HIGH ENERGY PHYS
[8]  
Auto D, 2004, J HIGH ENERGY PHYS
[9]  
Auto D, 2003, J HIGH ENERGY PHYS
[10]  
Baer H, 1999, PHYS REV D, V59, DOI 10.1103/PhysRevD.59.055014