Radiative corrections to aid the direct detection of the Higgsino-like neutralino dark matter: Spin-independent interactions

被引:3
作者
Bisal, Subhadip [1 ,2 ]
Chatterjee, Arindam [3 ]
Das, Debottam [1 ,2 ]
Pasha, Syed Adil [3 ]
机构
[1] Inst Phys, Bhubaneswer 751005, India
[2] Homi Bhabha Natl Inst, Training Sch Complex Anushakti Nagar, Mumbai 400094, India
[3] Shiv Nadar IoE Deemed be Univ, Gautam Buddha Nagar 201314, Uttar Pradesh, India
关键词
MISSING TRANSVERSE-MOMENTUM; ONE-LOOP CORRECTIONS; TEV PP COLLISIONS; ROOT-S=13 TEV; RELIC DENSITY; FINAL-STATES; PROGRAM; NATURALNESS; MICROMEGAS; CHARGINOS;
D O I
10.1103/PhysRevD.110.023043
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The lightest neutralino (chi 01) 0 1 ) is a good dark matter (DM) candidate in the R- parity conserving minimal supersymmetric Standard Model. In this work, we consider the light Higgsino-like neutralino as the lightest stable particle, thanks to a rather small Higgsino mass parameter . We then estimate the prominent radiative corrections to the neutralino-neutralino-Higgs boson vertices. We show that for Higgsino-like chi 01, 0 1 , these corrections can significantly influence the spin-independent direct detection cross section, even contributing close to 100% in certain regions of the parameter space. These corrections, therefore, play an important role in deducing constraints on the mass of the Higgsino-like lightest neutralino DM, and thus the parameter.
引用
收藏
页数:26
相关论文
共 115 条
[41]   Relic density at one-loop with gauge boson pair production [J].
Baro, N. ;
Boudjema, F. ;
Chalons, G. ;
Hao, Sun .
PHYSICAL REVIEW D, 2010, 81 (01)
[42]   Automatized full one-loop renormalization of the MSSM. II. The chargino-neutralino sector, the sfermion sector, and some applications [J].
Baro, N. ;
Boudjema, F. .
PHYSICAL REVIEW D, 2009, 80 (07)
[43]  
Beenakker W, 1997, NUCL PHYS B, V492, P51, DOI 10.1016/S0550-3213(97)00084-9
[44]   micrOMEGAs 2.0:: A program to calculate the relic density of dark matter in a generic model [J].
Belanger, G. ;
Boudjema, F. ;
Pukhov, A. ;
Semenov, A. .
COMPUTER PHYSICS COMMUNICATIONS, 2007, 176 (05) :367-382
[45]   micrOMEGAs:: Version 1.3 [J].
Bélanger, G ;
Boudjema, F ;
Pukhov, A ;
Semenov, A .
COMPUTER PHYSICS COMMUNICATIONS, 2006, 174 (07) :577-604
[46]   micrOMEGAs_3: A program for calculating dark matter observables [J].
Belanger, G. ;
Boudjema, F. ;
Pukhov, A. ;
Semenov, A. .
COMPUTER PHYSICS COMMUNICATIONS, 2014, 185 (03) :960-985
[47]   micrOMEGAs: A tool for dark matter studies [J].
Belanger, G. ;
Boudjema, F. ;
Pukhov, A. ;
Semenov, A. .
NUOVO CIMENTO C-COLLOQUIA AND COMMUNICATIONS IN PHYSICS, 2010, 33 (02) :111-116
[48]   Dark matter direct detection rate in a generic model with micrOMEGAs_2.2 [J].
Belanger, G. ;
Boudjema, F. ;
Pukhov, A. ;
Semenov, A. .
COMPUTER PHYSICS COMMUNICATIONS, 2009, 180 (05) :747-767
[49]   Particle dark matter: evidence, candidates and constraints [J].
Bertone, G ;
Hooper, D ;
Silk, J .
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 2005, 405 (5-6) :279-390
[50]  
Bisal S, 2024, Arxiv, DOI arXiv:2311.09938