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Your search keyword '"dark matter: relic density"' showing total 11 results
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11 results on '"dark matter: relic density"'

1. Indirect detection of secluded supersymmetric dark matter

Author

Patrick Barnes, Zachary Johnson, Aaron Pierce, and Bibhushan Shakya

Subjects
Astrophysics and Astronomy, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Cherenkov Telescope Array, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, mass [dark matter], Astrophysics::Cosmology and Extragalactic Astrophysics, annihilation [dark matter], gaugino, High Energy Physics - Phenomenology (hep-ph), dark matter: halo, emission [gamma ray], ddc:530, freeze-out: thermal, Particle Physics - Phenomenology, thermal [freeze-out], dark matter: relic density, dark matter: mass, High Energy Physics::Phenomenology, scale: electroweak interaction, hep-ph, halo [dark matter], dark matter: annihilation, electroweak interaction [scale], High Energy Physics - Phenomenology, gamma ray: emission, astro-ph.CO, relic density [dark matter], galaxy, supersymmetry, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

Physical review / D 105(3), 035005 (2022). doi:10.1103/PhysRevD.105.035005, Weak-scale secluded sector dark matter can reproduce the observed dark matter relic density with thermal freeze-out within that sector. If nature is supersymmetric, three portals to the visible sector���a gauge portal, a Higgs portal, and a gaugino portal���are present. We present gamma ray spectra relevant for indirect detection of dark matter annihilation in such setups. Since symmetries in the secluded sector can stabilize dark matter, R-parity is unnecessary, and we investigate the impact of R-parity violation on annihilation spectra. We present limits from the Fermi Large Area Telescope observations of dwarf galaxies and projections for Cherenkov Telescope Array observations of the galactic center. Many of our results are also applicable to generic, nonsupersymmetric setups., Published by Inst., Melville, NY

Published
2022
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2. WIMP Dark Matter in the U$\mu \nu$SSM

Author

Aguilar-Saavedra, J. A., López-Fogliani, D. E., Muñoz, C., and Pierre, Mathias

Subjects
High Energy Physics - Theory, supersymmetry and cosmology, neutrino: superfield, interpretation of experiments: CERN LHC Coll, dark matter, direct detection, quark: exotic, domain wall, dark matter: direct detection, neutrino, superfield, superpotential, WIMP: dark matter, dark matter [WIMP], High Energy Physics::Theory, U(1) [symmetry], superfield, singlet, ddc:530, singlet [superfield], structure, superfield: singlet, right-handed [neutrino], direct detection [dark matter], sneutrino, superfield [neutrino], neutrino, right-handed, dark matter theory, relic density, dark matter: relic density, WIMP, dark matter, High Energy Physics::Phenomenology, mediation [dark matter], symmetry: U(1), stability, quark, exotic, U(1), dark matter: mediation, High Energy Physics - Phenomenology, CERN LHC Coll, annihilation, particle physics - cosmology connection, neutrino: right-handed, exotic [quark], CERN LHC Coll [interpretation of experiments], relic density [dark matter], supersymmetry, hadronization, dark matter, mediation, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

Journal of cosmology and astroparticle physics 05(5), 004 (2022). doi:10.1088/1475-7516/2022/05/004, The U$\mu \nu$SSM is a U(1)' extension of the U$\mu \nu$SSM supersymmetric model, where baryon-number-violating operators as well as explicit mass terms are forbidden, and the potential domain wall problem is avoided. The gauge anomaly-cancellation conditions impose the presence of exotic quark superfields in the spectrum of U$\mu \nu$SSM models, and allow the presence of several singlet superfields under the standard model gauge group, in addition to the right-handed neutrino superfields. The gauge structure implies an additional discrete Z $_{2}$ symmetry in the superpotential, ensuring the stability of a singlet which behaves as WIMP dark matter without invoking R-parity. We analyze this novel possibility in detail, using the fermionic component of the singlet as the dark matter candidate. In particular, we compute its amount of relic density via Z', Higgs-right sneutrino and dark matter mediated annihilations, and its potential signals in dark matter direct detection experiments. The constraints on the parameter space due to Z'; direct searches at the LHC are imposed in the analysis, as well as those from the hadronization inside the detector of the exotic quarks. Large regions of the parameter space turn out to be in the reach of the upcoming Darwin experiment., Published by IOP, London

Published
2022
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3. String Fragmentation in Supercooled Confinement and implications for Dark Matter

Author

Baldes, Iason, Gouttenoire, Yann, and Sala, Filippo

Subjects
flux, dark matter: composite, dark matter: relic density, deep inelastic scattering, bubble, confinement, string: fragmentation, scale: confinement, Lorentz, plasma
Abstract

A strongly-coupled sector can feature a supercooled confinement transition in the early universe. We point out that, when fundamental quanta of the strong sector are swept into expanding bubbles of the confined phase, the distance between them is large compared to the confinement scale. The flux linking the fundamental quanta then deforms and stretches towards the wall, producing an enhanced number of composite states upon string fragmentation. The composite states are highly boosted in the plasma frame, which leads to additional particle production through the subsequent deep inelastic scattering. We propose a modelling of these dynamics and study the consequences for the abundance and energetics of particles in the universe and for bubble-wall Lorentz factors. This opens several new avenues of investigation, which we begin to explore here, showing that the composite dark matter relic density is affected by many orders of magnitude.

Published
2021
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4. Reconciling Higgs physics and pseudo-Nambu-Goldstone dark matter in the S2HDM using a genetic algorithm

Author

Biekoetter, Thomas and Olea Romacho, Maria Olalla

Subjects
Higgs Physics, CMS, dark matter: relic density, dark matter: mass, potential: scalar, scattering, bottom: pair production, CERN LEP Stor, Goldstone particle, Higgs particle: doublet, vacuum: stability, Beyond Standard Model, direct detection, final state: two-photon, freeze-out: thermal
Abstract

doi:10.1007/JHEP10(2021)215, We investigate a possible realization ofpseudo-Nambu-Goldstone (pNG) dark matterin the framework of a singlet-extended 2 Higgsdoublet model (S2HDM). pNG dark matter gainedattraction due to the fact that direct-detectionconstraints can be avoided naturally because of themomentum-suppressed scattering cross sections,whereas the relic abundance of dark matter cannevertheless be accounted for via the usual thermalfreeze-out mechanism. We confront the S2HDM witha multitude of theoretical and experimentalconstraints, paying special attention to thetheoretical limitations on the scalar potential,such as vacuum stability and perturbativity.In addition, we discussthe complementarity between constraintsrelated to the dark matter sector, on theone hand, and to the Higgs sector, on the other hand.In our numerical discussion we explore theHiggs funnel region with dark mattermasses around 60GeV using a genetic algorithm.We demonstrate that the S2HDM can easilyaccount for the measured relic abundance whilebeing in agreement with all relevant constraints.We also discuss whether the so-calledcenter-of-galaxy excesses can beaccommodated,possibly incombination with a Higgsboson at about 96GeV that can be the originof the LEP- and the CMS-excess observed at this massin the $b \bar b$-quark andthe diphoton final state, respectively.

Published
2021
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5. WIMP Dark Matter in the U$\mu \nu$SSM

Author

Aguilar-Saavedra, J. A., López-Fogliani, D. E., Muñoz, C., and Pierre, M.

Subjects
supersymmetry and cosmology, neutrino: superfield, interpretation of experiments: CERN LHC Coll, dark matter, direct detection, quark: exotic, domain wall, dark matter: direct detection, neutrino, superfield, superpotential, WIMP: dark matter, High Energy Physics::Theory, superfield, singlet, structure, superfield: singlet, sneutrino, dark matter theory, neutrino, right-handed, relic density, dark matter: relic density, High Energy Physics::Phenomenology, WIMP, dark matter, symmetry: U(1), stability, quark, exotic, U(1), dark matter: mediation, CERN LHC Coll, annihilation, particle physics - cosmology connection, neutrino: right-handed, supersymmetry, hadronization, dark matter, mediation
Abstract

The U$\mu\nu$SSM is a $U(1)'$ extension of the $\mu\nu$SSM supersymmetric model, where baryon-number-violating operators as well as explicit mass terms are forbidden, and the potential domain wall problem is avoided. The gauge anomaly-cancellation conditions impose the presence of exotic quark superfields in the spectrum of U$\mu\nu$SSM models, and allow the presence of several singlet superfields under the standard model gauge group, in addition to the right-handed neutrino superfields. The gauge structure implies an additional discrete $Z_2$ symmetry in the superpotential, ensuring the stability of a singlet which behaves as WIMP dark matter without invoking $R$-parity. We analyze this novel possibility in detail, using the fermionic component of the singlet as the dark matter candidate. In particular, we compute its amount of relic density via $Z'$, Higgs-right sneutrino and dark matter mediated annihilations, and its potential signals in dark matter direct detection experiments. The constraints on the parameter space due to $Z'$ direct searches at the LHC are imposed in the analysis, as well as those from the hadronization inside the detector of the exotic quarks. Large regions of the parameter space turn out to be in the reach of the upcoming Darwin experiment.

Published
2021
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6. Combination and summary of ATLAS dark matter searches using 139 fb$^{-1}$ of $\sqrt {s}$ = 13 TeV $p p$ collision data and interpreted in a two-Higgs-doublet model with a pseudoscalar mediator

Author

ATLAS Collaboration

Subjects
dark matter: interaction, Yukawa [coupling], 13000 GeV-cms, branching ratio: upper limit, branching ratio [Higgs particle], mass [dark matter], coupling: scalar, WIMP: dark matter, dark matter [WIMP], dark matter: coupling, axial-vector [coupling], benchmark, scattering [p p], Dark Matter, pair production [dark matter], doublet [Higgs particle], new physics: search for, transverse energy: missing-energy, dark matter: pair production, 2HDMa, ATLAS, mass dependence, channel cross section: branching ratio: upper limit, pair production [bottom], CERN LHC Coll, EXOTICS, lower limit [mass], relic density [dark matter], colliding beams [p p], interaction [dark matter], signature, p p: scattering, mass: lower limit, Higgs particle: invisible decay, parameter space [supersymmetry], bottom: pair production, vector [coupling], Higgs particle: doublet, coupling [dark matter], search for [new physics], dark matter: associated production, coupling: pseudoscalar, branching ratio: upper limit [channel cross section], coupling: vector, dark matter: relic density, dark matter: mass, mediation [dark matter], supersymmetry: parameter space, leptonic decay [Z0], pseudoscalar [coupling], coupling: axial-vector, dark matter: mediation, Higgs particle: branching ratio, scalar [coupling], missing-energy [transverse energy], hadronic decay [Higgs particle], Higgs particle: hadronic decay, Z0: leptonic decay, upper limit [branching ratio], High Energy Physics::Experiment, associated production [dark matter], p p: colliding beams, coupling: Yukawa, invisible decay [Higgs particle], experimental results
Abstract

29 pp. (2021)., A combination of two searches for dark matter is presented, along with results from a wide range of experimental analyses that are interpreted in a common benchmark model: a Two-Higgs-Doublet Model with a pseudoscalar mediator. The analyses use up to 139 fb$^{-1}$ of proton-proton collision data at a centre-of-mass energy $\sqrt{s}=13$ TeV recorded with the ATLAS detector at the LHC between 2015-2018. The results from two searches targeting the $E_T^{\textrm{miss}}+Z(\ell\ell)$ and $E_T^{\textrm{miss}}+h(b\bar{b})$ signatures are statistically combined. The constraints of a wide range of additional experimental analyses, targeting final states with and without invisible particles, are evaluated and summarised alongside the combination in several interpretations within this model.

Published
2021
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7. Constraining the Inert Doublet Model using Vector Boson Fusion

Author

Tania Robens and Daniel Dercks

Subjects
Particle physics, Physics and Astronomy (miscellaneous), Physics of Elementary Particles and Fields, Dark matter, Scalar (mathematics), single production [jet], FOS: Physical sciences, lcsh:Astrophysics, Parameter space, Lambda, fusion [vector boson], mass: scalar, 01 natural sciences, dark matter, Vector boson, Higgs particle: doublet, Two-Higgs-doublet model, High Energy Physics - Phenomenology (hep-ph), vector boson: fusion, 0103 physical sciences, lcsh:QB460-466, ddc:530, lcsh:Nuclear and particle physics. Atomic energy. Radioactivity, scalar [mass], 010306 general physics, Engineering (miscellaneous), dark-matter, Higgs-boson, symmetry-breaking, physics, search, collisions, bounds, Physics, Fusion, doublet [Higgs particle], 010308 nuclear & particles physics, dark matter: relic density, High Energy Physics::Phenomenology, jet: single production, sensitivity, High Energy Physics - Phenomenology, Higgs boson, lcsh:QC770-798, relic density [dark matter], High Energy Physics::Experiment
Abstract

The European physical journal / C 79(11), 924 (2019). doi:10.1140/epjc/s10052-019-7436-6, In this work, we use a recast of the Run II search for invisible Higgs decays within Vector Boson Fusion to constrain the parameter space of the Inert Doublet model, a two Higgs doublet model with a dark matter candidate. When including all known theoretical as well as collider constraints, we find that the above can rule out a relatively large part in the $m_H,\,\lambda _{345}$ parameter space, for dark scalar masses $m_H\,\le \,100\,{\mathrm{GeV}}$. Including the latest dark matter constraints, a smaller part of parameter space remains which is solely excluded from the above analysis. We also discuss the sensitivity of monojet searches and multilepton final states from Run II., Published by Springer, Heidelberg

Published
2018
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8. Dark Matter Freeze-out During Matter Domination

Author

Hamdan, Saleh and Unwin, James

Subjects
dark matter: coupling, new physics, dark matter: relic density, dark matter: mass, nucleosynthesis: big bang, dark matter: freeze-out
Abstract

Modern physics letters / A 33(29), 1850181 (2018). doi:10.1142/S021773231850181X, We highlight the general scenario of dark matter freeze-out while the energy density of the universe is dominated by a decoupled non-relativistic species. Decoupling during matter domination changes the freeze-out dynamics, since the Hubble rate is parametrically different for matter and radiation domination. Furthermore, for successful Big Bang Nucleosynthesis the state dominating the early universe energy density must decay, this dilutes (or repopulates) the dark matter. As a result, the masses and couplings required to reproduce the observed dark matter relic density can differ significantly from radiation-dominated freeze-out., Published by World Scientific Publ., Singapur

Published
2018
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9. Dark matter models for the 511 keV galactic line predict keV electron recoils on Earth

Author

Ema, Yohei, Sala, Filippo, and Sato, Ryosuke

Subjects
observatory, accelerator, 13. Climate action, electron: recoil, photon: emission, dark matter: relic density, dark matter: annihilation, galaxy, 7. Clean energy
Abstract

The European physical journal / C 81(2), 129 (1-6) (2021). doi:10.1140/epjc/s10052-021-08899-y, We propose models of Dark Matter that account for the 511 keV photon emission from the Galactic Centre, compatibly with experimental constraints and theoretical consistency, and where the relic abundance is achieved via $p$-wave annihilations or, in inelastic models, via co-annihilations. Due to the Dark Matter component that is inevitably upscattered by the Sun, these models generically predict keV electron recoils at detectors on Earth, and could naturally explain the excess recently reported by the XENON1T collaboration. The very small number of free parameters make these ideas testable by detectors like XENONnT and Panda-X, by accelerators like NA64 and LDMX, and by cosmological surveys like the Simons observatory and CMB-S4. As a byproduct of our study, we recast NA64 limits on invisibly decaying dark photons to other particles., Published by Springer, Heidelberg

10. Self-interacting dark matter with a stable vector mediator

Author

Duerr, Michael, Schmidt-Hoberg, Kai, and Wild, Sebastian

Subjects
dark matter: coupling, dark matter: interaction, new physics, dark matter: relic density, nucleosynthesis: big bang, Astrophysics::Cosmology and Extragalactic Astrophysics, dark matter: freeze-out, cosmic background radiation, 7. Clean energy, freeze-out: thermal, dark matter: mediation
Abstract

Light vector mediators can naturally induce velocity-dependent dark matter self-interactions while at the same time allowing for the correct dark matter relic abundance via thermal freeze-out. If these mediators subsequently decay into Standard Model states such as electrons or photons however, this is robustly excluded by constraints from the Cosmic Microwave Background. We study to what extent this conclusion can be circumvented if the vector mediator is stable and hence contributes to the dark matter density while annihilating into lighter degrees of freedom. We find viable parts of parameter space which lead to the desired self-interaction cross section of dark matter to address the small-scale problems of the collisionless cold dark matter paradigm while being compatible with bounds from the Cosmic Microwave Background and Big Bang Nucleosynthesis observations.

11. Search for dark matter produced in association with bottom or top quarks in $\sqrt{s}$ = 13 TeV pp collisions with the ATLAS detector

Author

Aaboud, Morad, Aad, Georges, Abbott, Brad, Abdinov, Ovsat, Abeloos, Baptiste, Abidi, Syed Haider, AbouZeid, Ossama, Abraham, Nicola, Abramowicz, Halina, Abreu, Henso, Abreu, Ricardo, Abulaiti, Yiming, Acharya, Bobby Samir, Adachi, Shunsuke, Adamczyk, Leszek, Adelman, Jahred, Adersberger, Michael, Adye, Tim, Affolder, Tony, Afik, Yoav, Agatonovic-Jovin, Tatjana, Agheorghiesei, Catalin, Aguilar-Saavedra, Juan Antonio, Ahlen, Steven, Ahmadov, Faig, Aielli, Giulio, Akatsuka, Shunichi, Akerstedt, Henrik, Åkesson, Torsten Paul Ake, Akilli, Ece, Akimov, Andrei, Alberghi, Gian Luigi, Albert, Justin, Albicocco, Pietro, Alconada Verzini, Maria Josefina, Alderweireldt, Sara, Aleksa, Martin, Aleksandrov, Igor, Alexa, Calin, Alexander, Gideon, Alexopoulos, Theodoros, Alhroob, Muhammad, Ali, Babar, Aliev, Malik, Alimonti, Gianluca, Alison, John, Alkire, Steven Patrick, Allbrooke, Benedict, Allen, Benjamin William, Allport, Phillip, Aloisio, Alberto, Alonso, Alejandro, Alonso, Francisco, Alpigiani, Cristiano, Alshehri, Azzah Aziz, Alstaty, Mahmoud, Alvarez Gonzalez, Barbara, Άlvarez Piqueras, Damián, Alviggi, Mariagrazia, Amadio, Brian Thomas, Amaral Coutinho, Yara, Amelung, Christoph, Amidei, Dante, Amor Dos Santos, Susana Patricia, Amoroso, Simone, Anastopoulos, Christos, Ancu, Lucian Stefan, Andari, Nansi, Andeen, Timothy, Anders, Christoph Falk, Anders, John Kenneth, Anderson, Kelby, Andreazza, Attilio, Andrei, George Victor, Angelidakis, Stylianos, Angelozzi, Ivan, Angerami, Aaron, Anisenkov, Alexey, Anjos, Nuno, Annovi, Alberto, Antel, Claire, Antonelli, Mario, Antonov, Alexey, Antrim, Daniel Joseph, Anulli, Fabio, Aoki, Masato, Aperio Bella, Ludovica, Arabidze, Giorgi, Arai, Yasuo, Araque, Juan Pedro, Araujo Ferraz, Victor, Arce, Ayana, Ardell, Rose Elisabeth, Arduh, Francisco Anuar, Arguin, Jean-Francois, Argyropoulos, Spyridon, Arik, Metin, Armbruster, Aaron James, Armitage, Lewis James, Arnaez, Olivier, Arnold, Hannah, Arratia, Miguel, Arslan, Ozan, Artamonov, Andrei, Artoni, Giacomo, Artz, Sebastian, Asai, Shoji, Asbah, Nedaa, Ashkenazi, Adi, Asquith, Lily, Assamagan, Ketevi, Astalos, Robert, Atkinson, Markus, Atlay, Naim Bora, Augsten, Kamil, Avolio, Giuseppe, Axen, Bradley, Ayoub, Mohamad Kassem, Azuelos, Georges, Baas, Alessandra, Baca, Matthew John, Bachacou, Henri, Bachas, Konstantinos, Backes, Moritz, Bagnaia, Paolo, Bahmani, Marzieh, Bahrasemani, Sina, Baines, John, Bajic, Milena, Baker, Oliver Keith, Bakker, Pepijn Johannes, Baldin, Evgenii, Balek, Petr, Balli, Fabrice, Balunas, William Keaton, Banas, Elzbieta, Bandyopadhyay, Anjishnu, Banerjee, Swagato, Bannoura, Arwa A E, Barak, Liron, Barberio, Elisabetta Luigia, Barberis, Dario, Barbero, Marlon, Barillari, Teresa, Barisits, Martin-Stefan, Barkeloo, Jason Tyler Colt, Barklow, Timothy, Barlow, Nick, Barnes, Sarah Louise, Barnett, Bruce, Barnett, Michael, Barnovska-Blenessy, Zuzana, Baroncelli, Antonio, Barone, Gaetano, Barr, Alan, Barranco Navarro, Laura, Barreiro, Fernando, Barreiro Guimarães Da Costa, João, Bartoldus, Rainer, Barton, Adam Edward, Bartos, Pavol, Basalaev, Artem, Bassalat, Ahmed, Bates, Richard, Batista, Santiago Juan, Batley, Richard, Battaglia, Marco, Bauce, Matteo, Bauer, Florian, Bawa, Harinder Singh, Beacham, James, Beattie, Michael David, Beau, Tristan, Beauchemin, Pierre-Hugues, Bechtle, Philip, Beck, Hans~Peter, Beck, Helge Christoph, Becker, Kathrin, Becker, Maurice, Becot, Cyril, Beddall, Andrew, Beddall, Ayda, Bednyakov, Vadim, Bedognetti, Matteo, Bee, Christopher, Beermann, Thomas, Begalli, Marcia, Begel, Michael, Behr, Janna Katharina, Bell, Andrew Stuart, Bella, Gideon, Bellagamba, Lorenzo, Bellerive, Alain, Bellomo, Massimiliano, Belotskiy, Konstantin, Beltramello, Olga, Belyaev, Nikita, Benary, Odette, Benchekroun, Driss, Bender, Michael, Benekos, Nektarios, Benhammou, Yan, Benhar Noccioli, Eleonora, Benitez, Jose, Benjamin, Douglas, Benoit, Mathieu, Bensinger, James, Bentvelsen, Stan, Beresford, Lydia, Beretta, Matteo, Berge, David, Bergeaas Kuutmann, Elin, Berger, Nicolas, Bergsten, Laura Jean, Beringer, Jürg, Berlendis, Simon, Bernard, Nathan Rogers, Bernardi, Gregorio, Bernius, Catrin, Bernlochner, Florian Urs, Berry, Tracey, Berta, Peter, Bertella, Claudia, Bertoli, Gabriele, Bertram, Iain Alexander, Bertsche, Carolyn, Besjes, Geert-Jan, Bessidskaia Bylund, Olga, Bessner, Martin Florian, Besson, Nathalie, Bethani, Agni, Bethke, Siegfried, Betti, Alessandra, Bevan, Adrian John, Beyer, Julien-Christopher, Bianchi, Riccardo-Maria, Biebel, Otmar, Biedermann, Dustin, Bielski, Rafal, Bierwagen, Katharina, Biesuz, Nicolo Vladi, Biglietti, Michela, Billoud, Thomas Remy Victor, Bilokon, Halina, Bindi, Marcello, Bingul, Ahmet, Bini, Cesare, Biondi, Silvia, Bisanz, Tobias, Bittrich, Carsten, Bjergaard, David Martin, Black, James, Black, Kevin, Blair, Robert, Blazek, Tomas, Bloch, Ingo, Blocker, Craig, Blue, Andrew, Blumenschein, Ulrike, Blunier, Sylvain, Bobbink, Gerjan, Bobrovnikov, Victor, Bocchetta, Simona Serena, Bocci, Andrea, Bock, Christopher, Boehler, Michael, Boerner, Daniela, Bogavac, Danijela, Bogdanchikov, Alexander, Bohm, Christian, Boisvert, Veronique, Bokan, Petar, Bold, Tomasz, Boldyrev, Alexey, Bolz, Arthur Eugen, Bomben, Marco, Bona, Marcella, Boonekamp, Maarten, Borisov, Anatoly, Borissov, Guennadi, Bortfeldt, Jonathan, Bortoletto, Daniela, Bortolotto, Valerio, Boscherini, Davide, Bosman, Martine, Bossio Sola, Jonathan David, Boudreau, Joseph, Bouhova-Thacker, Evelina Vassileva, Boumediene, Djamel Eddine, Bourdarios, Claire, Boutle, Sarah Kate, Boveia, Antonio, Boyd, James, Boyko, Igor, Bozson, Adam James, Bracinik, Juraj, Brandt, Andrew, Brandt, Gerhard, Brandt, Oleg, Braren, Frued, Bratzler, Uwe, Brau, Benjamin, Brau, James, Breaden Madden, William Dmitri, Brendlinger, Kurt, Brennan, Amelia Jean, Brenner, Lydia, Brenner, Richard, Bressler, Shikma, Briglin, Daniel Lawrence, Bristow, Timothy Michael, Britton, Dave, Britzger, Daniel, Brochu, Frederic, Brock, Ian, Brock, Raymond, Brooijmans, Gustaaf, Brooks, Timothy, Brooks, William, Brosamer, Jacquelyn, Brost, Elizabeth, Broughton, James, Bruckman De Renstrom, Pawel, Bruncko, Dusan, Bruni, Alessia, Bruni, Graziano, Bruni, Lucrezia Stella, Bruno, Salvatore, Brunt, Benjamin, Bruschi, Marco, Bruscino, Nello, Bryant, Patrick, Bryngemark, Lene, Buanes, Trygve, Buat, Quentin, Buchholz, Peter, Buckley, Andrew, Budagov, Ioulian, Buehrer, Felix, Bugge, Magnar Kopangen, Bulekov, Oleg, Bullock, Daniel, Burch, Tyler James, Burdin, Sergey, Burgard, Carsten Daniel, Burger, Angela Maria, Burghgrave, Blake, Burka, Klaudia, Burke, Stephen, Burmeister, Ingo, Burr, Jonathan Thomas Peter, Büscher, Daniel, Büscher, Volker, Bussey, Peter, Butler, John, Buttar, Craig, Butterworth, Jonathan, Butti, Pierfrancesco, Buttinger, William, Buzatu, Adrian, Buzykaev, Aleksey, C-Q, Changqiao, Cabrera Urbán, Susana, Caforio, Davide, Cai, Huacheng, Cairo, Valentina, Cakir, Orhan, Calace, Noemi, Calafiura, Paolo, Calandri, Alessandro, Calderini, Giovanni, Calfayan, Philippe, Callea, Giuseppe, Caloba, Luiz, Calvente Lopez, Sergio, Calvet, David, Calvet, Samuel, Calvet, Thomas Philippe, Camacho Toro, Reina, Camarda, Stefano, Camarri, Paolo, Cameron, David, Caminal Armadans, Roger, Camincher, Clement, Campana, Simone, Campanelli, Mario, Camplani, Alessandra, Campoverde, Angel, Canale, Vincenzo, Cano Bret, Marc, Cantero, Josu, Cao, Tingting, Capeans Garrido, Maria Del Mar, Caprini, Irinel, Caprini, Mihai, Capua, Marcella, Carbone, Ryne Michael, Cardarelli, Roberto, Cardillo, Fabio, Carli, Ina, Carli, Tancredi, Carlino, Gianpaolo, Carlson, Benjamin Taylor, Carminati, Leonardo, Carney, Rebecca, Caron, Sascha, Carquin, Edson, Carrá, Sonia, Carrillo-Montoya, German D, Casadei, Diego, Casado, Maria Pilar, Casha, Albert Francis, Casolino, Mirkoantonio, Casper, David William, Castelijn, Remco, Castillo Gimenez, Victoria, Castro, Nuno Filipe, Catinaccio, Andrea, Catmore, James, Cattai, Ariella, Caudron, Julien, Cavaliere, Viviana, Cavallaro, Emanuele, Cavalli, Donatella, Cavalli-Sforza, Matteo, Cavasinni, Vincenzo, Celebi, Emre, Ceradini, Filippo, Cerda Alberich, Leonor, Santiago Cerqueira, Augusto, Cerri, Alessandro, Cerrito, Lucio, Cerutti, Fabio, Cervelli, Alberto, Cetin, Serkant Ali, Chafaq, Aziz, Chakraborty, Dhiman, Chan, Stephen Kam-Wah, Chan, Wing Sheung, Chan, Yat Long, Chang, Philip, Chapman, John Derek, Charlton, Dave, Chau, Chav Chhiv, Chavez Barajas, Carlos Alberto, Che, Siinn, Cheatham, Susan, Chegwidden, Andrew, Chekanov, Sergei, Chekulaev, Sergey, Chelkov, Gueorgui, Chelstowska, Magda Anna, Chen, Cheng, Chen, Chunhui, Chen, Hucheng, Chen, Jing, Chen, Shenjian, Chen, Shion, Chen, Xin, Chen, Ye, Cheng, Hok Chuen, Cheng, Huajie, Cheplakov, Alexander, Cheremushkina, Evgeniya, Cherkaoui El Moursli, Rajaa, Cheu, Elliott, Cheung, Kingman, Chevalier, Laurent, Chiarella, Vitaliano, Chiarelli, Giorgio, Chiodini, Gabriele, Chisholm, Andrew, Chitan, Adrian, Chiu, Yu Him Justin, Chizhov, Mihail, Choi, Kyungeon, Chomont, Arthur Rene, Chouridou, Sofia, Chow, Yun Sang, Christodoulou, Valentinos, Chu, Ming Chung, Chudoba, Jiri, Chuinard, Annabelle Julia, Chwastowski, Janusz, Chytka, Ladislav, Ciftci, Abbas Kenan, Cinca, Diane, Cindro, Vladimir, Cioara, Irina Antonela, Ciocio, Alessandra, Cirotto, Francesco, Citron, Zvi Hirsh, Citterio, Mauro, Ciubancan, Mihai, Clark, Allan G, Clark, Brian Lee, Clark, Michael, Clark, Philip James, Clarke, Robert, Clement, Christophe, Coadou, Yann, Cobal, Marina, Coccaro, Andrea, Cochran, James H, Colasurdo, Luca, Cole, Brian, Colijn, Auke-Pieter, Collot, Johann, Colombo, Tommaso, Conde Muiño, Patricia, Coniavitis, Elias, Connell, Simon Henry, Connelly, Ian, Constantinescu, Serban, Conti, Geraldine, Conventi, Francesco, Cooke, Mark, Cooper-Sarkar, Amanda, Cormier, Felix, Cormier, Kyle James Read, Corradi, Massimo, Corriveau, Francois, Cortes-Gonzalez, Arely, Costa, Giuseppe, Costa, María José, Costanzo, Davide, Cottin, Giovanna, Cowan, Glen, Cox, 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Giulia, Ristić, Branislav, Ritsch, Elmar, Riu, Imma, Rizatdinova, Flera, Rizvi, Eram, Rizzi, Chiara, Roberts, Rhys Thomas, Robertson, Steven, Robichaud-Veronneau, Andree, Robinson, Dave, Robinson, James, Robson, Aidan, Rocco, Elena, Roda, Chiara, Rodina, Yulia, Rodriguez Bosca, Sergi, Rodriguez Perez, Andrea, Rodriguez Rodriguez, Daniel, Roe, Shaun, Rogan, Christopher Sean, Røhne, Ole, Roloff, Jennifer, Romaniouk, Anatoli, Romano, Marino, Romano Saez, Silvestre Marino, Romero Adam, Elena, Rompotis, Nikolaos, Ronzani, Manfredi, Roos, Lydia, Rosati, Stefano, Rosbach, Kilian, Rose, Peyton, Rosien, Nils-Arne, Rossi, Elvira, Rossi, Leonardo Paolo, Rosten, Jonatan, Rosten, Rachel, Rotaru, Marina, Rothberg, Joseph, Rousseau, David, Roy, Debarati, Rozanov, Alexandre, Rozen, Yoram, Ruan, Xifeng, Rubbo, Francesco, Rühr, Frederik, Ruiz-Martinez, Aranzazu, Rurikova, Zuzana, Rusakovich, Nikolai, Russell, Heather, Rutherfoord, John, Ruthmann, Nils, Rüttinger, Elias Michael, Ryabov, Yury, Rybar, 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S., Sultansoy, Saleh, Sumida, Toshi, Sun, Siyuan, Sun, Xiaohu, Suruliz, Kerim, Suster, Carl, Sutton, Mark, Suzuki, Shota, Svatos, Michal, Swiatlowski, Maximilian, Swift, Stewart Patrick, Sykora, Ivan, Sykora, Tomas, Ta, Duc, Tackmann, Kerstin, Taenzer, Joe, Taffard, Anyes, Tafirout, Reda, Tahirovic, Elvedin, Taiblum, Nimrod, Takai, Helio, Takashima, Ryuichi, Takasugi, Eric Hayato, Takeda, Kosuke, Takeshita, Tohru, Takubo, Yosuke, Talby, Mossadek, Talyshev, Alexey, Tanaka, Junichi, Tanaka, Masahiro, Tanaka, Reisaburo, Tanaka, Shuji, Tanioka, Ryo, Tannenwald, Benjamin Bordy, Tapia Araya, Sebastian, Tapprogge, Stefan, Tarem, Shlomit, Tartarelli, Giuseppe Francesco, Tas, Petr, Tasevsky, Marek, Tashiro, Takuya, Tassi, Enrico, Tavares Delgado, Ademar, Tayalati, Yahya, Taylor, Aaron, Taylor, Alan James, Taylor, Geoffrey, Taylor, Pierre Thor Elliot, Taylor, Wendy, Teixeira-Dias, Pedro, Temple, Darren, Ten Kate, Herman, Teng, Ping-Kun, Teoh, Jia Jian, Tepel, Fabian-Phillipp, Terada, Susumu, Terashi, Koji, Terron, Juan, Terzo, Stefano, Testa, Marianna, Teuscher, Richard, Thais, Savannah Jennifer, Theveneaux-Pelzer, Timothée, Thiele, Fabian, Thomas, Juergen, Thomas-Wilsker, Joshuha, Thompson, Paul, Thompson, Stan, Thomsen, Lotte Ansgaard, Thomson, Evelyn, Tian, Yun, Tibbetts, Mark James, Ticse Torres, Royer Edson, Tikhomirov, Vladimir, Tikhonov, Yury, Timoshenko, Sergey, Tipton, Paul, Tisserant, Sylvain, Todome, Kazuki, Todorova-Nova, Sharka, Todt, Stefanie, Tojo, Junji, Tokár, Stanislav, Tokushuku, Katsuo, Tolley, Emma, Tomlinson, Lee, Tomoto, Makoto, Tompkins, Lauren, Toms, Konstantin, Tornambe, Peter, Torrence, Eric, Torres, Heberth, Torró Pastor, Emma, Toth, Jozsef, Touchard, Francois, Tovey, Daniel, Treado, Colleen Jennifer, Trefzger, Thomas, Tresoldi, Fabio, Tricoli, Alessandro, Trigger, Isabel Marian, Trincaz-Duvoid, Sophie, Tripiana, Martin, Trischuk, William, Trocmé, Benjamin, Trofymov, Artur, Troncon, Clara, Trottier-McDonald, Michel, Trovatelli, Monica, Truong, 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Subjects
p p: scattering, transverse momentum: missing-energy, final state: ((n)jet), background, 13000 GeV-cms, dark matter: mass, dark matter: relic density, mass: lower limit, family: 3, coupling: scalar, ATLAS, 7. Clean energy, WIMP: dark matter, channel cross section: upper limit, dark matter: mediation, CERN LHC Coll, unitarity, sbottom, coupling: pseudoscalar, p p: colliding beams, stop: associated production, experimental results
Abstract

The European physical journal / C 78(1), 18 (2018). doi:10.1140/epjc/s10052-017-5486-1, A search for weakly interacting massive dark-matter particles produced in association with bottom or top quarks is presented. Final states containing third-generation quarks and missing transverse momentum are considered. The analysis uses $36.1 \, \mathrm {fb}^{-1}$ of proton–proton collision data recorded by the ATLAS experiment at $\sqrt{s}=13$ TeV in 2015 and 2016. No significant excess of events above the estimated backgrounds is observed. The results are interpreted in the framework of simplified models of spin-0 dark-matter mediators. For colour-neutral spin-0 mediators produced in association with top quarks and decaying into a pair of dark-matter particles, mediator masses below 50 GeV are excluded assuming a dark-matter candidate mass of 1 GeV and unitary couplings. For scalar and pseudoscalar mediators produced in association with bottom quarks, the search sets limits on the production cross-section of 300 times the predicted rate for mediators with masses between 10 and $50\, \hbox {GeV}$ and assuming a dark-matter mass of $1 \,\hbox {GeV}$ and unitary coupling. Constraints on colour-charged scalar simplified models are also presented. Assuming a dark-matter particle mass of $35\, \hbox {GeV}$ , mediator particles with mass below $1.1\, \hbox {TeV}$ are excluded for couplings yielding a dark-matter relic density consistent with measurements., Published by Springer, Berlin

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