Search for vector mediator of dark matter production in invisible decay mode; Physical Review D; Vol. 97, iss. 7

Detalles Bibliográficos
Parent link:Physical Review D: covering particles, fields, gravitation, and cosmology
Vol. 97, iss. 7.— 2018.— [072002, 22 p.]
Autor Corporativo: Национальный исследовательский Томский политехнический университет Исследовательская школа физики высокоэнергетических процессов
Outros autores: Banerjee D., Crivelli P. Paolo, Burtsev V. E. Vitaly Evgenjevich, Chumakov A. G. Aleksandr Grigorjevich, Dusaev R. R. Renat Ramilyevich, Lyubovitskiy (Lyubovitskij) V. E. Valery Efimovich, Trifonov A. Yu. Andrey Yurievich, Vasilishin B. I. Bogdan Ivanovich
Summary:Title screen
A search is performed for a new sub-GeV vector boson (A′) mediated production of dark matter (χ) in the fixed-target experiment, NA64, at the CERN SPS. The A′, called dark photon, can be generated in the reaction e−Z→e−ZA′ of 100 GeV electrons dumped against an active target followed by its prompt invisible decay A′→χ¯χ. The experimental signature of this process would be an event with an isolated electron and large missing energy in the detector. From the analysis of the data sample collected in 2016 corresponding to 4.3×1010 electrons on target no evidence of such a process has been found. New stringent constraints on the A′ mixing strength with photons, 10−5≲ε≲10−2, for the A′ mass range mA′≲1  GeV are derived. For models considering scalar and fermionic thermal dark matter interacting with the visible sector through the vector portal the 90% C.L. limits 10−11≲y≲10−6on the dark-matter parameter y=ε2αD(mχmA′)4 are obtained for the dark coupling constant αD=0.5and dark-matter masses 0.001≲mχ≲0.5  GeV. The lower limits αD≳10−3 for pseudo-Dirac dark matter in the mass region mχ≲0.05  GeV are more stringent than the corresponding bounds from beam dump experiments. The results are obtained by using exact tree level calculations of the A′production cross sections, which turn out to be significantly smaller compared to the one obtained in the Weizsäcker-Williams approximation for the mass region mA′≳0.1  GeV
Idioma:inglés
Publicado: 2018
Subjects:
Acceso en liña:http://earchive.tpu.ru/handle/11683/57565
https://doi.org/10.1103/PhysRevD.97.072002
Formato: Electrónico Capítulo de libro
KOHA link:https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=660075

MARC

LEADER 00000naa0a2200000 4500
001 660075
005 20251106105615.0
035 |a (RuTPU)RU\TPU\network\28997 
090 |a 660075 
100 |a 20190422d2018 k||y0rusy50 ba 
101 0 |a eng 
102 |a US 
135 |a drcn ---uucaa 
181 0 |a i  
182 0 |a b 
200 1 |a Search for vector mediator of dark matter production in invisible decay mode  |f D. Banerjee [et al.] 
203 |a Text  |c electronic 
300 |a Title screen 
320 |a [References: 76 tit.] 
330 |a A search is performed for a new sub-GeV vector boson (A′) mediated production of dark matter (χ) in the fixed-target experiment, NA64, at the CERN SPS. The A′, called dark photon, can be generated in the reaction e−Z→e−ZA′ of 100 GeV electrons dumped against an active target followed by its prompt invisible decay A′→χ¯χ. The experimental signature of this process would be an event with an isolated electron and large missing energy in the detector. From the analysis of the data sample collected in 2016 corresponding to 4.3×1010 electrons on target no evidence of such a process has been found. New stringent constraints on the A′ mixing strength with photons, 10−5≲ε≲10−2, for the A′ mass range mA′≲1  GeV are derived. For models considering scalar and fermionic thermal dark matter interacting with the visible sector through the vector portal the 90% C.L. limits 10−11≲y≲10−6on the dark-matter parameter y=ε2αD(mχmA′)4 are obtained for the dark coupling constant αD=0.5and dark-matter masses 0.001≲mχ≲0.5  GeV. The lower limits αD≳10−3 for pseudo-Dirac dark matter in the mass region mχ≲0.05  GeV are more stringent than the corresponding bounds from beam dump experiments. The results are obtained by using exact tree level calculations of the A′production cross sections, which turn out to be significantly smaller compared to the one obtained in the Weizsäcker-Williams approximation for the mass region mA′≳0.1  GeV 
461 |t Physical Review D  |o covering particles, fields, gravitation, and cosmology 
463 |t Vol. 97, iss. 7  |v [072002, 22 p.]  |d 2018 
610 1 |a электронный ресурс 
610 1 |a труды учёных ТПУ 
610 1 |a нелептонные распады 
610 1 |a векторные методы 
610 1 |a медиаторы 
701 1 |a Banerjee  |b D. 
701 1 |a Crivelli  |b P.  |g Paolo 
701 1 |a Burtsev  |b V. E.  |c mathematician  |c Senior Lecturer of Tomsk Polytechnic University  |f 1991-  |g Vitaly Evgenjevich  |3 (RuTPU)RU\TPU\pers\38282 
701 1 |a Chumakov  |b A. G.  |c physicist  |c laboratory assistant-researcher of Tomsk Polytechnic University  |f 1992-  |g Aleksandr Grigorjevich  |3 (RuTPU)RU\TPU\pers\41079 
701 1 |a Dusaev  |b R. R.  |c specialist in the field of nuclear physics  |c Engineer of Tomsk Polytechnic University  |f 1988-  |g Renat Ramilyevich  |3 (RuTPU)RU\TPU\pers\30972  |9 15210 
701 1 |a Lyubovitskiy (Lyubovitskij)  |b V. E.  |c physicist  |c Professor of Tomsk Polytechnic University, Doctor of physical and mathematical sciences, Professor of the University of Tubingen (Germany)  |f 1963-  |g Valery Efimovich  |3 (RuTPU)RU\TPU\pers\33385  |9 17080 
701 1 |a Trifonov  |b A. Yu.  |c physicist, mathematician  |c Professor of Tomsk Polytechnic University, Doctor of physical and mathematical sciences  |f 1963-  |g Andrey Yurievich  |3 (RuTPU)RU\TPU\pers\30754 
701 1 |a Vasilishin  |b B. I.  |c engineer-physicist  |c laboratory researcher at Tomsk Polytechnic University  |f 1990-  |g Bogdan Ivanovich  |3 (RuTPU)RU\TPU\pers\37572  |9 20428 
712 0 2 |a Национальный исследовательский Томский политехнический университет  |b Исследовательская школа физики высокоэнергетических процессов  |c (2017- )  |3 (RuTPU)RU\TPU\col\23551 
801 2 |a RU  |b 63413507  |c 20220207  |g RCR 
856 4 |u http://earchive.tpu.ru/handle/11683/57565 
856 4 |u https://doi.org/10.1103/PhysRevD.97.072002 
942 |c CF