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A thorough analysis of sneutrinos as dark matter candidates is performed, in different classes of supersymmetric models, as is typically done for the neutralino dark matter. First in the Minimal Supersymmetric Standard Model, sneutrinos are…

High Energy Physics - Phenomenology · Physics 2008-05-15 Chiara Arina

In supersymmetric extensions of the Standard Model, the lightest neutralino, the gravitino, and the axino can appear as the lightest supersymmetric particle and as such provide a compelling explanation of the non-baryonic dark matter in our…

High Energy Physics - Phenomenology · Physics 2007-11-28 Frank Daniel Steffen

We consider a class of models involving interactions between ultra-light scalar dark matter and Standard Model neutrinos. Such couplings modify the neutrino mass splittings and mixing angles to include additional components that vary in…

High Energy Physics - Phenomenology · Physics 2016-12-07 Asher Berlin

The lightest neutralino in supersymmetric models with conserved R-parity is an attractive candidate for non-luminous matter in the universe. If relic neutralinos are indeed present as dark matter in our galaxy, they can be directly detected…

High Energy Physics - Phenomenology · Physics 2007-05-23 Michal Brhlik

Recent proposals have suggested that a previously unknown decay mode of the neutron into a dark matter particle could solve the long lasting measurement problem of the neutron decay width. We show that, if the dark particle in neutron decay…

Nuclear Theory · Physics 2018-11-09 T. F. Motta , P. A. M. Guichon , A. W. Thomas

The multi-ton-scale liquid xenon detectors, with an excellent energy resolution of a few keV, will be constructed to probe the dark-matter particles. In this paper, we show that precision measurements of the low-energy solar neutrinos via…

High Energy Physics - Phenomenology · Physics 2019-02-15 Guo-yuan Huang , Shun Zhou

Phenomenology of neutralino dark matter in the minimal supersymmetric model is discussed for a scenario where the lightest Higgs boson mass is lighter than 114.4 GeV. We show that the scenario is consistent not only with many collider…

High Energy Physics - Phenomenology · Physics 2008-11-26 Masaki Asano , Shigeki Matsumoto , Masato Senami , Hiroaki Sugiyama

One method to search for particle dark matter is to hunt down its annihilation products. In the Solar System, three potential types of signals of annihilation have been identified: neutrinos and gamma-rays from the Sun, and neutrinos from…

High Energy Astrophysical Phenomena · Physics 2009-05-19 Annika H. G. Peter

Neutrino telescopes have a wide scientic scope. One of their main goals is the detection of dark matter, for which they have specic advantages. Neutrino telescopes offer the possibility of looking at several kinds of sources, not all of…

High Energy Astrophysical Phenomena · Physics 2017-10-11 J. D. Zornoza , C. Toennis

We consider the neutralino as a dominant Dark Matter particle in the galactic halo and investigate some general issues of direct Dark Matter searches via elastic neutralino-nucleus scattering. On the basis of conventional assumptions about…

High Energy Physics - Phenomenology · Physics 2007-05-23 V. A. Bednyakov , H. V. Klapdor-Kleingrothaus , S. G. Kovalenko

The majority of the matter in the universe is still unidentified and under investigation by both direct and indirect means. Many experiments searching for the recoil of dark-matter particles off target nuclei in underground laboratories…

High Energy Physics - Phenomenology · Physics 2015-10-28 Michael Klasen , Martin Pohl , Günter Sigl

If the dark matter in the Universe is made of weakly self-interacting particles, they may self-annihilate and emit gamma-rays. We use high resolution numerical simulations to estimate directly the annihilation flux from the central regions…

Astrophysics · Physics 2009-09-25 Felix Stoehr , Simon D. M. White , Volker Springel , Giuseppe Tormen , Naoki Yoshida

Dark matter particles annihilating in the Galactic halo can provide a flux of positrons potentially observable in upcoming experiments, such as PAMELA and AMS-02. We discuss the spectral features which may be associated with dark matter…

High Energy Physics - Phenomenology · Physics 2009-11-10 Dan Hooper , Joseph Silk

How large can the dark matter self-annihilation rate in the late universe be? This rate depends on (rho_DM/m_chi)^2 <sigma_A v>, where rho_DM/m_chi is the number density of dark matter, and the annihilation cross section is averaged over…

Astrophysics · Physics 2008-11-26 John F. Beacom

As cosmology has entered a phase of precision experiments, the content of the universe has been established to contain interesting and not yet fully understood components, namely dark energy and dark matter. While the cause and exact nature…

High Energy Physics - Phenomenology · Physics 2015-06-25 Lars Bergstrom

We discuss JUNO sensitivity to the annihilation of MeV dark matter in the galactic halo via detecting inverse beta decay reactions of electron anti-neutrinos resulting from the annihilation. We study possible backgrounds to the signature,…

High Energy Physics - Experiment · Physics 2023-09-15 JUNO Collaboration , Angel Abusleme , Thomas Adam , Shakeel Ahmad , Rizwan Ahmed , Sebastiano Aiello , Muhammad Akram , Abid Aleem , Tsagkarakis Alexandros , Fengpeng An , Qi An , Giuseppe Andronico , Nikolay Anfimov , Vito Antonelli , Tatiana Antoshkina , Burin Asavapibhop , João Pedro Athayde Marcondes de André , Didier Auguste , Weidong Bai , Nikita Balashov , Wander Baldini , Andrea Barresi , Davide Basilico , Eric Baussan , Marco Bellato , Antonio Bergnoli , Daniel Bick , Thilo Birkenfeld , Sylvie Blin , David Blum , Simon Blyth , Anastasia Bolshakova , Mathieu Bongrand , Clément Bordereau , Dominique Breton , Augusto Brigatti , Riccardo Brugnera , Riccardo Bruno , Antonio Budano , Jose Busto , Ilya Butorov , Anatael Cabrera , Barbara Caccianiga , Hao Cai , Xiao Cai , Yanke Cai , Zhiyan Cai , Riccardo Callegari , Antonio Cammi , Agustin Campeny , Chuanya Cao , Guofu Cao , Jun Cao , Rossella Caruso , Cédric Cerna , Chi Chan , Jinfan Chang , Yun Chang , Guoming Chen , Pingping Chen , Po-An Chen , Shaomin Chen , Yixue Chen , Yu Chen , Zhiyuan Chen , Zikang Chen , Jie Cheng , Yaping Cheng , Yu Chin Cheng , Alexander Chepurnov , Alexey Chetverikov , Davide Chiesa , Pietro Chimenti , Ziliang Chu , Artem Chukanov , Gérard Claverie , Catia Clementi , Barbara Clerbaux , Marta Colomer Molla , Selma Conforti Di Lorenzo , Daniele Corti , Flavio Dal Corso , Olivia Dalager , Christophe De La Taille , Zhi Deng , Ziyan Deng , Wilfried Depnering , Marco Diaz , Xuefeng Ding , Yayun Ding , Bayu Dirgantara , Sergey Dmitrievsky , Tadeas Dohnal , Dmitry Dolzhikov , Georgy Donchenko , Jianmeng Dong , Evgeny Doroshkevich , Wei Dou , Marcos Dracos , Frédéric Druillole , Ran Du , Shuxian Du , Stefano Dusini , Martin Dvorak , Jessica Eck , Timo Enqvist , Andrea Fabbri , Ulrike Fahrendholz , Donghua Fan , Lei Fan , Jian Fang , Wenxing Fang , Marco Fargetta , Dmitry Fedoseev , Zhengyong Fei , Li-Cheng Feng , Qichun Feng , Richard Ford , Amélie Fournier , Haonan Gan , Feng Gao , Alberto Garfagnini , Arsenii Gavrikov , Marco Giammarchi , Nunzio Giudice , Maxim Gonchar , Guanghua Gong , Hui Gong , Yuri Gornushkin , Alexandre Göttel , Marco Grassi , Maxim Gromov , Vasily Gromov , Minghao Gu , Xiaofei Gu , Yu Gu , Mengyun Guan , Yuduo Guan , Nunzio Guardone , Cong Guo , Wanlei Guo , Xinheng Guo , Yuhang Guo , Caren Hagner , Ran Han , Yang Han , Miao He , Wei He , Tobias Heinz , Patrick Hellmuth , Yuekun Heng , Rafael Herrera , YuenKeung Hor , Shaojing Hou , Yee Hsiung , Bei-Zhen Hu , Hang Hu , Jianrun Hu , Jun Hu , Shouyang Hu , Tao Hu , Yuxiang Hu , Zhuojun Hu , Guihong Huang , Hanxiong Huang , Kaixuan Huang , Wenhao Huang , Xin Huang , Xingtao Huang , Yongbo Huang , Jiaqi Hui , Lei Huo , Wenju Huo , Cédric Huss , Safeer Hussain , Ara Ioannisian , Roberto Isocrate , Beatrice Jelmini , Ignacio Jeria , Xiaolu Ji , Huihui Jia , Junji Jia , Siyu Jian , Di Jiang , Wei Jiang , Xiaoshan Jiang , Xiaoping Jing , Cécile Jollet , Leonidas Kalousis , Philipp Kampmann , Li Kang , Rebin Karaparambil , Narine Kazarian , Amina Khatun , Khanchai Khosonthongkee , Denis Korablev , Konstantin Kouzakov , Alexey Krasnoperov , Nikolay Kutovskiy , Pasi Kuusiniemi , Tobias Lachenmaier , Cecilia Landini , Sébastien Leblanc , Victor Lebrin , Frederic Lefevre , Ruiting Lei , Rupert Leitner , Jason Leung , Daozheng Li , Demin Li , Fei Li , Fule Li , Gaosong Li , Huiling Li , Mengzhao Li , Min Li , Nan Li , Nan Li , Qingjiang Li , Ruhui Li , Rui Li , Shanfeng Li , Tao Li , Teng Li , Weidong Li , Weiguo Li , Xiaomei Li , Xiaonan Li , Xinglong Li , Yi Li , Yichen Li , Yufeng Li , Zepeng Li , Zhaohan Li , Zhibing Li , Ziyuan Li , Zonghai Li , Hao Liang , Hao Liang , Jiajun Liao , Ayut Limphirat , Guey-Lin Lin , Shengxin Lin , Tao Lin , Jiajie Ling , Ivano Lippi , Fang Liu , Haidong Liu , Haotian Liu , Hongbang Liu , Hongjuan Liu , Hongtao Liu , Hui Liu , Jianglai Liu , Jinchang Liu , Min Liu , Qian Liu , Qin Liu , Runxuan Liu , Shubin Liu , Shulin Liu , Xiaowei Liu , Xiwen Liu , Yan Liu , Yunzhe Liu , Alexey Lokhov , Paolo Lombardi , Claudio Lombardo , Kai Loo , Chuan Lu , Haoqi Lu , Jingbin Lu , Junguang Lu , Peizhi Lu , Shuxiang Lu , Bayarto Lubsandorzhiev , Sultim Lubsandorzhiev , Livia Ludhova , Arslan Lukanov , Daibin Luo , Fengjiao Luo , Guang Luo , Shu Luo , Wuming Luo , Xiaojie Luo , Vladimir Lyashuk , Bangzheng Ma , Bing Ma , Qiumei Ma , Si Ma , Xiaoyan Ma , Xubo Ma , Jihane Maalmi , Jingyu Mai , Yury Malyshkin , Roberto Carlos Mandujano , Fabio Mantovani , Xin Mao , Yajun Mao , Stefano M. Mari , Filippo Marini , Gisele Martin-Chassard , Agnese Martini , Matthias Mayer , Davit Mayilyan , Ints Mednieks , Artur Meinusch , Yue Meng , Anselmo Meregaglia , Emanuela Meroni , David Meyhöfer , Mauro Mezzetto , Jonathan Miller , Lino Miramonti , Paolo Montini , Michele Montuschi , Axel Müller , Massimiliano Nastasi , Dmitry V. Naumov , Elena Naumova , Diana Navas-Nicolas , Igor Nemchenok , Minh Thuan Nguyen Thi , Alexey Nikolaev , Feipeng Ning , Zhe Ning , Hiroshi Nunokawa , Lothar Oberauer , Juan Pedro Ochoa-Ricoux , Alexander Olshevskiy , Domizia Orestano , Fausto Ortica , Rainer Othegraven , Alessandro Paoloni , Sergio Parmeggiano , Yatian Pei , Luca Pelicci , Anguo Peng , Haiping Peng , Yu Peng , Zhaoyuan Peng , Frédéric Perrot , Pierre-Alexandre Petitjean , Fabrizio Petrucci , Oliver Pilarczyk , Luis Felipe Piñeres Rico , Artyom Popov , Pascal Poussot , Ezio Previtali , Fazhi Qi , Ming Qi , Sen Qian , Xiaohui Qian , Zhen Qian , Hao Qiao , Zhonghua Qin , Shoukang Qiu , Gioacchino Ranucci , Reem Rasheed , Alessandra Re , Henning Rebber , Abdel Rebii , Mariia Redchuk , Bin Ren , Jie Ren , Barbara Ricci , Mariam Rifai , Mathieu Roche , Narongkiat Rodphai , Aldo Romani , Bedřich Roskovec , Xichao Ruan , Arseniy Rybnikov , Andrey Sadovsky , Paolo Saggese , Simone Sanfilippo , Anut Sangka , Utane Sawangwit , Julia Sawatzki , Michaela Schever , Cédric Schwab , Konstantin Schweizer , Alexandr Selyunin , Andrea Serafini , Giulio Settanta , Mariangela Settimo , Zhuang Shao , Vladislav Sharov , Arina Shaydurova , Jingyan Shi , Yanan Shi , Vitaly Shutov , Andrey Sidorenkov , Fedor Šimkovic , Chiara Sirignano , Jaruchit Siripak , Monica Sisti , Maciej Slupecki , Mikhail Smirnov , Oleg Smirnov , Thiago Sogo-Bezerra , Sergey Sokolov , Julanan Songwadhana , Boonrucksar Soonthornthum , Albert Sotnikov , Ondřej Šrámek , Warintorn Sreethawong , Achim Stahl , Luca Stanco , Konstantin Stankevich , Dušan Štefánik , Hans Steiger , Jochen Steinmann , Tobias Sterr , Matthias Raphael Stock , Virginia Strati , Alexander Studenikin , Jun Su , Shifeng Sun , Xilei Sun , Yongjie Sun , Yongzhao Sun , Zhengyang Sun , Narumon Suwonjandee , Michal Szelezniak , Jian Tang , Qiang Tang , Quan Tang , Xiao Tang , Vidhya Thara Hariharan , Eric Theisen , Alexander Tietzsch , Igor Tkachev , Tomas Tmej , Marco Danilo Claudio Torri , Konstantin Treskov , Andrea Triossi , Giancarlo Troni , Wladyslaw Trzaska , Yu-Chen Tung , Cristina Tuve , Nikita Ushakov , Vadim Vedin , Giuseppe Verde , Maxim Vialkov , Benoit Viaud , Cornelius Moritz Vollbrecht , Cristina Volpe , Katharina von Sturm , Vit Vorobel , Dmitriy Voronin , Lucia Votano , Pablo Walker , Caishen Wang , Chung-Hsiang Wang , En Wang , Guoli Wang , Jian Wang , Jun Wang , Lu Wang , Meifen Wang , Meng Wang , Meng Wang , Ruiguang Wang , Siguang Wang , Wei Wang , Wei Wang , Wenshuai Wang , Xi Wang , Xiangyue Wang , Yangfu Wang , Yaoguang Wang , Yi Wang , Yi Wang , Yifang Wang , Yuanqing Wang , Yuman Wang , Zhe Wang , Zheng Wang , Zhimin Wang , Zongyi Wang , Apimook Watcharangkool , Wei Wei , Wei Wei , Wenlu Wei , Yadong Wei , Kaile Wen , Liangjian Wen , Jun Weng , Christopher Wiebusch , Bjoern Wonsak , Diru Wu , Qun Wu , Zhi Wu , Michael Wurm , Jacques Wurtz , Christian Wysotzki , Yufei Xi , Dongmei Xia , Xiang Xiao , Xiaochuan Xie , Yuguang Xie , Zhangquan Xie , Zhao Xin , Zhizhong Xing , Benda Xu , Cheng Xu , Donglian Xu , Fanrong Xu , Hangkun Xu , Jilei Xu , Jing Xu , Meihang Xu , Yin Xu , Yu Xu , Baojun Yan , Qiyu Yan , Taylor Yan , Wenqi Yan , Xiongbo Yan , Yupeng Yan , Changgen Yang , Chengfeng Yang , Huan Yang , Jie Yang , Lei Yang , Xiaoyu Yang , Yifan Yang , Yifan Yang , Haifeng Yao , Jiaxuan Ye , Mei Ye , Ziping Ye , Frédéric Yermia , Zhengyun You , Boxiang Yu , Chiye Yu , Chunxu Yu , Hongzhao Yu , Miao Yu , Xianghui Yu , Zeyuan Yu , Zezhong Yu , Cenxi Yuan , Chengzhuo Yuan , Ying Yuan , Zhenxiong Yuan , Baobiao Yue , Noman Zafar , Vitalii Zavadskyi , Shan Zeng , Tingxuan Zeng , Yuda Zeng , Liang Zhan , Aiqiang Zhang , Bin Zhang , Binting Zhang , Feiyang Zhang , Guoqing Zhang , Honghao Zhang , Jialiang Zhang , Jiawen Zhang , Jie Zhang , Jin Zhang , Jingbo Zhang , Jinnan Zhang , Mohan Zhang , Peng Zhang , Qingmin Zhang , Shiqi Zhang , Shu Zhang , Tao Zhang , Xiaomei Zhang , Xin Zhang , Xuantong Zhang , Yinhong Zhang , Yiyu Zhang , Yongpeng Zhang , Yu Zhang , Yuanyuan Zhang , Yumei Zhang , Zhenyu Zhang , Zhijian Zhang , Jie Zhao , Rong Zhao , Runze Zhao , Shujun Zhao , Dongqin Zheng , Hua Zheng , Yangheng Zheng , Weirong Zhong , Jing Zhou , Li Zhou , Nan Zhou , Shun Zhou , Tong Zhou , Xiang Zhou , Jingsen Zhu , Kangfu Zhu , Kejun Zhu , Zhihang Zhu , Bo Zhuang , Honglin Zhuang , Liang Zong , Jiaheng Zou , Sebastian Zwickel

Sterile neutrinos may be one of the best Warm Dark Matter candidates we have today. Both lower and upper bounds on the mass of the sterile neutrino come from astronomical observations. We show that the proper inclusion of the neutrino…

Astrophysics · Physics 2008-11-26 Steen H. Hansen , Julien Lesgourgues , Sergio Pastor , Joseph Silk

Dark matter halos contain a wealth of substructure in the form of subhalos and tidal streams. Enhancements in the dark matter density of these regions leads to enhanced rates in direct detection experiments, as well as enhanced dark matter…

High Energy Astrophysical Phenomena · Physics 2009-12-09 Savvas M. Koushiappas , Marc Kamionkowski

Exotic dark matter together with dark energy or cosmological constant seem to dominate in the Universe. An even higher density of such matter seems to be gravitationally trapped in our Galaxy. The nature of dark matter can be unveiled only,…

Nuclear Theory · Physics 2009-09-29 J. D. Vergados

We point out that with improving our present knowledge of experimental neutrino physics it will be possible to locate nuclear powered vehicles like submarines, aircraft carriers and UFOs and detect nuclear testing. Since neutrinos cannot be…

High Energy Physics - Phenomenology · Physics 2007-05-23 P. Panigrahi , U. Sarkar
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