David Curtin, Kaustubh Deshpande, Oliver Fischer, Jose Zurita
The future electron-proton collider proposals, LHeC and FCC-he, can deliver $\mathcal{O}$(TeV) center-of-mass energy collisions, higher than most of the proposed lepton accelerators, with $\mathcal{O}$(ab$^{-1}$) luminosity, while maintaining a much cleaner experimental environment as compared to the hadron machines. This unique capability of $e^- p$ colliders can be harnessed in probing BSM scenarios giving final states that look like hadronic noise at $pp$ machines. In the present study, we explore the prospects of detecting such a prompt signal having multiple soft jets at the LHeC. Such a signal can come from the decay of gluino in RPV or Stealth SUSY, where there exists a gap in the current experimental search with $m_{\tilde{g}} \approx 50 - 70$ GeV. We perform a simple analysis to demonstrate that, with simple signal selection cuts, we can close this gap at the LHeC at 95 % confidence level, even in the presence of a reasonable systematic error. More sophisticated signal selection strategies and detailed knowledge of the detector can be used to improve the prospects of signal detection.
Malte Buschmann, Sonia El Hedri, Anna Kaminska, Jia Liu, Maikel de Vries, Xiao-Ping Wang, Felix Yu, Jose Zurita
Simplified models of the dark matter (co)annihilation mechanism predict striking new collider signatures untested by current searches. These models, which were codified in the coannihilation codex, provide the basis for a dark matter (DM) discovery program at the Large Hadron Collider (LHC) driven by the measured DM relic density. In this work, we study an exemplary model featuring $s$-channel DM coannihilation through a scalar diquark mediator as a representative case study of scenarios with strongly interacting coannihilation partners. We discuss the full phenomenology of the model, ranging from low energy flavor constraints, vacuum stability requirements, and precision Higgs effects to direct detection and indirect detection prospects. Moreover, motivated by the relic density calculation, we find significant portions of parameter space are compatible with current collider constraints and can be probed by future searches, including a proposed analysis for the novel signature of a dijet resonance accompanied by missing transverse energy (MET). Our results show that the $13$ TeV LHC with $100~\mathrm{fb}^{-1}$ luminosity should be sensitive to mediators as heavy as 1 TeV and dark matter in the 400--500 GeV range. The combination of searches for single and paired dijet peaks, non-resonant jets + MET excesses, and our novel resonant dijet + MET signature have strong coverage of the motivated relic density region, reflecting the tight connections between particles determining the dark matter abundance and their experimental signatures at the LHC.
Rakhi Mahbubani, Pedro Schwaller, Jose Zurita
We investigate the sensitivity at current and future hadron colliders to a heavy electrically-charged particle with a proper decay length below a centimetre, whose decay products are invisible due to below-threshold energies and/or small couplings to the Standard Model. A cosmologically-motivated example of a framework that contains such a particle is the Minimal Supersymmetric Standard Model in the limit of pure Higgsinos. The current hadron-collider search strategy has no sensitivity to the upper range of pure Higgsino masses that are consistent with the thermal relic density, even at a future collider with 100 TeV centre-of-mass energy. We show that performing a disappearing track search within the inner 10 cm of detector volume would improve the reach in lifetime by a factor of 3 at the 14 TeV LHC and a further factor of 5 at a 100 TeV collider, resulting in around 10 events for 1.1 TeV thermal Higgsinos. In order to include the particles with the largest boost in the analysis, we furthermore propose a purely track-based search in both the central and forward regions, each of which would increase the number of events by another factor of 5, improving our reach at small lifetimes. This would allow us to definitively discover or exclude the experimentally-elusive pure-Higgsino thermal relic at a 100 TeV collider.
Chiara Aimè, Aram Apyan, Mohammed Attia Mahmoud, Nazar Bartosik, Alessandro Bertolin, Maurizio Bonesini, Salvatore Bottaro, Dario Buttazzo, Rodolfo Capdevilla, Massimo Casarsa, Luca Castelli, Maria Gabriella Catanesi, Francesco Giovanni Celiberto, Alessandro Cerri, Cari Cesarotti, Grigorios Chachamis, Siyu Chen, Yang-Ting Chien, Mauro Chiesa, Gianmaria Collazuol, Marco Costa, Nathaniel Craig, David Curtin, Sridhara Dasu, Jorge De Blas, Dmitri Denisov, Haluk Denizli, Radovan Dermisek, Luca Di Luzio, Biagio Di Micco, Keith Dienes, Tommaso Dorigo, Anna Ferrari, Davide Fiorina, Roberto Franceschini, Francesco Garosi, Alfredo Glioti, Mario Greco, Admir Greljo, Ramona Groeber, Christophe Grojean, Jiayin Gu, Tao Han, Brian Henning, Keith Hermanek, Tova Ray Holmes, Samuel Homiller, Sudip Jana, Sergo Jindariani, Yonatan Kahn, Ivan Karpov, Wolfgang Kilian, Kyoungchul Kong, Patrick Koppenburg, Karol Krizka, Lawrence Lee, Qiang Li, Ronald Lipton, Zhen Liu, Kenneth Long, Ian Low, Donatella Lucchesi, Yang Ma, Lianliang Ma, Fabio Maltoni, Bruno Mansoulie, Luca Mantani, David Marzocca, Navin McGinnis, Barbara Mele, Federico Meloni, Claudia Merlassino, Alessandro Montella, Marco Nardecchia, Federico Nardi, Paolo Panci, Simone Pagan Griso, Giuliano Panico, Rocco Paparella, Paride Paradisi, Nadia Pastrone, Fulvio Piccinini, Karolos Potamianos, Emilio Radicioni, Riccardo Rattazzi, Diego Redigolo, Laura Reina, Jürgen Reuter, Cristina Riccardi, Lorenzo Ricci, Ursula van Rienen, Luciano Ristori, Tania Natalie Robens, Richard Ruiz, Filippo Sala, Jakub Salko, Paola Salvini, Ennio Salvioni, Daniel Schulte, Michele Selvaggi, Abdulkadir Senol, Lorenzo Sestini, Varun Sharma, Jing Shu, Rosa Simoniello, Giordon Holtsberg Stark, Daniel Stolarski, Shufang Su, Wei Su, Olcyr Sumensari, Xiaohu Sun, Raman Sundrum, Jian Tang, Andrea Tesi, Brooks Thomas, Riccardo Torre, Sokratis Trifinopoulos, Ilaria Vai, Alessandro Valenti, Ludovico Vittorio, Liantao Wang, Yongcheng Wu, Andrea Wulzer, Xiaoran Zhao, Jose Zurita
The perspective of designing muon colliders with high energy and luminosity, which is being investigated by the International Muon Collider Collaboration, has triggered a growing interest in their physics reach. We present a concise summary of the muon colliders potential to explore new physics, leveraging on the unique possibility of combining high available energy with very precise measurements.
Rakhi Mahbubani, Jose Zurita
We examine the sensitivity at a future 100 TeV proton-proton collider to compressed dark sectors whose decay products are invisible due to below-threshold energies and/or small couplings to the Standard Model. This scenario could be relevant to models of WIMP dark matter, where the lightest New Physics state is an (isolated) electroweak multiplet whose lowest component is stable on cosmological timescales. We rely on the additional emission of a hard on-shell $Z$-boson decaying to leptons, a channel with low background systematics, and include a careful estimate of the real and fake backgrounds to this process in our analysis. We show that an integrated luminosity of 30 ab$^{-1}$ would allow exclusion of a TeV-scale compressed dark sector with inclusive production cross section of 0.3 fb, for 1\% background systematic uncertainty and splittings below 5 GeV. This translates to exclusion of a pure higgsino (wino) multiplet with mass of 500 (970) GeV.
Erich Weihs, Jose Zurita
We study how collider data and electroweak precision observables affect the parameter space of models including a new dark force mediated by a massive U(1) gauge boson. It acquires mass via a Higgs mechanism in the dark sector which is connected to the Standard Model through kinetic mixing of the two U(1) gauge bosons and the Higgs potential. We assess the impact of the 7 TeV LHC and show that most of the parameter space of the model can be probed with an integrated luminosity of 15 fb^-1.
Florian Goertz, Andreas Papaefstathiou, Li Lin Yang, José Zurita
We consider the ratio of cross sections of double-to-single Higgs boson production at the Large Hadron Collider at 14 TeV. Since both processes possess similar higher-order corrections, leading to a cancellation of uncertainties in the ratio, this observable is well-suited to constrain the trilinear Higgs boson self-coupling. We consider the scale variation, parton density function uncertainties and conservative estimates of experimental uncertainties, applied to the viable decay channels, to construct expected exclusion regions. We show that the trilinear self-coupling can be constrained to be positive with a 600/fb LHC dataset at 95% confidence level. Moreover, we demonstrate that we expect to obtain a ~+30% and ~-20 uncertainty on the self-coupling at 3000/fb without statistical fitting of differential distributions. The present article outlines the most precise method of determination of the Higgs trilinear coupling to date.
Branden Aitken, Cristiano Alpigiani, Juan Carlos Arteaga-Velázquez, Mitchel Baker, Kincso Balazs, Jared Barron, Brian Batell, Austin Batz, Yan Benhammou, Tamara Alice Bud, Karen Salomé Caballero-Mora, John Paul Chou, David Curtin, Albert de Roeck, Miriam Diamond, Mariia Didenko, Keith R. Dienes, William Dougherty, Liam Andrew Dougherty, Marco Drewes, Sameer Erramilli, Erez Etzion, Arturo Fernández Téllez, Grace Finlayson, Oliver Fischer, Jim Freeman, Jonathan Gall, Ali Garabaglu, Bhawna Gomber, Stephen Elliott Greenberg, Jaipratap Singh Grewal, Zoe Hallman, Bahgat Hassan, Yuekun Heng, Keegan Humphrey, Trystan Humphrey, Graham D. Kribs, Alex Lau, Jiahao Liao, Zhen Liu, Giovanni Marsella, Matthew McCullough, David McKeen, Patrick Meade, Caleb Miller, Gilad Mizrachi, O. G. Morales-Olivares, David Morrissey, Abdulrahman Ahmed Morsy, John Osborn, Gabriel Owh, Michalis Panagiotou, Mason Proffitt, Runze Ren, Steven H. Robertson, Mario Rodríguez-Cahuantzi, Heather Russell, Victoria Sánchez, Halil Saka, Mamoksh Samra, Rodney Schnarr, Jessie Shelton, Yiftah Silver, Daniel Stolarski, Martin A. Subieta Vasquez, Sanjay Kumar Swain, Steffie Ann Thayil, Brooks Thomas, Emma Torro, Yuhsin Tsai, Bennett Winnicky-Lewis, Igor Zolkin, Jose Zurita
We present the Conceptual Design Report (CDR) for the MATHUSLA (MAssive Timing Hodoscope for Ultra-Stable neutraL pArticles) long-lived particle detector at the HL-LHC, covering the design, fabrication and installation at CERN Point 5. MATHUSLA is a 40 m-scale detector with an air-filled decay volume that is instrumented with scintillator tracking detectors, to be located near CMS. Its large size, close proximity to the CMS interaction point and about 100 m of rock shielding from HL-LHC backgrounds allows it to detect LLP production rates and lifetimes that are one to two orders of magnitude beyond the ultimate sensitivity of the HL-LHC main detectors for many highly motivated LLP signals. Data taking is projected to commence with the start of HL-LHC operations. We present a new 40m design for the detector: its individual scintillator bars and wavelength-shifting fibers, their organization into tracking layers, tracking modules, tower modules and the veto detector; define a high-level design for the supporting electronics, DAQ and trigger system, including supplying a hardware trigger signal to CMS to record the LLP production event; outline computing systems, civil engineering and safety considerations; and present preliminary cost estimates and timelines for the project. We also conduct detailed simulation studies of the important cosmic ray and HL-LHC muon backgrounds, implementing full track/vertex reconstruction and background rejection, to ultimately demonstrate high signal efficiency and $\ll 1$ background event in realistic LLP searches for the main physics targets at MATHUSLA. This sensitivity is robust with respect to detector design or background simulation details. Appendices provide various supplemental information.
Cristiano Alpigiani, Juan Carlos Arteaga-Velázquez, Austin Ball, Liron Barak, Jared Barron, Brian Batell, James Beacham, Yan Benhammo, Karen Salomé Caballero-Mora, Paolo Camarri, Roberto Cardarelli, John Paul Chou, Wentao Cui, David Curtin, Miriam Diamond, Keith R. Dienes, Liam Andrew Dougherty, Giuseppe Di Sciascio, Marco Drewes, Erez Etzion, Rouven Essig, Jared Evans, Arturo Fernández Téllez, Oliver Fischer, Jim Freeman, Jonathan Gall, Ali Garabaglu, Stefano Giagu, Stephen Elliott Greenberg, Bhawna Gomber, Roberto Guida, Andy Haas, Yuekun Heng, Shih-Chieh Hsu, Giuseppe Iaselli, Ken Johns, Audrey Kvam, Dragoslav Lazic, Liang Li, Barbara Liberti, Zhen Liu, Henry Lubatti, Lillian Luo, Giovanni Marsella, Mario Iván Martínez Hernández, Matthew McCullough, David McKeen, Patrick Meade, Gilad Mizrachi, O. G. Morales-Olivares, David Morrissey, Meny Raviv Moshe, Antonio Policicchio, Mason Proffitt, Dennis Cazar Ramirez, Matthew Reece, Steven H. Robertson, Mario Rodríguez-Cahuantzi, Albert de Roeck, Amber Roepe, Joe Rothberg, James John Russell, Heather Russell, Rinaldo Santonico, Marco Schioppa, Jessie Shelton, Brian Shuve, Yiftah Silver, Luigi Di Stante, Daniel Stolarski, Mike Strauss, David Strom, John Stupak, Martin A. Subieta Vasquez, Sanjay Kumar Swain, Guillermo Tejeda Muñoz, Steffie Ann Thayil, Brooks Thomas, Yuhsin Tsai, Emma Torro, Gordon Watts, Charles Young, Jose Zurita
We report on recent progress in the design of the proposed MATHUSLA Long Lived Particle (LLP) detector for the HL-LHC, updating the information in the original Letter of Intent (LoI), see CDS:LHCC-I-031, arXiv:1811.00927. A suitable site has been identified at LHC Point 5 that is closer to the CMS Interaction Point (IP) than assumed in the LoI. The decay volume has been increased from 20 m to 25 m in height. Engineering studies have been made in order to locate much of the decay volume below ground, bringing the detector even closer to the IP. With these changes, a 100 m x 100 m detector has the same physics reach for large c$τ$ as the 200 m x 200 m detector described in the LoI and other studies. The performance for small c$τ$ is improved because of the proximity to the IP. Detector technology has also evolved while retaining the strip-like sensor geometry in Resistive Plate Chambers (RPC) described in the LoI. The present design uses extruded scintillator bars read out using wavelength shifting fibers and silicon photomultipliers (SiPM). Operations will be simpler and more robust with much lower operating voltages and without the use of greenhouse gases. Manufacturing is straightforward and should result in cost savings. Understanding of backgrounds has also significantly advanced, thanks to new simulation studies and measurements taken at the MATHUSLA test stand operating above ATLAS in 2018. We discuss next steps for the MATHUSLA collaboration, and identify areas where new members can make particularly important contributions.
Marcela Carena, Kyoungchul Kong, Eduardo Ponton, Jose Zurita
We consider supersymmetric models that include particles beyond the Minimal Supersymmetric Standard Model (MSSM) with masses in the TeV range, and that couple significantly to the MSSM Higgs sector. We perform a model-independent analysis of the spectrum and couplings of the MSSM Higgs fields, based on an effective theory of the MSSM degrees of freedom. The tree-level mass of the lightest CP-even state can easily be above the LEP bound of 114 GeV, thus allowing for a relatively light spectrum of superpartners, restricted only by direct searches. The Higgs spectrum and couplings can be significantly modified compared to the MSSM ones, often allowing for interesting new decay modes. We also observe that the gluon fusion production cross section of the SM-like Higgs can be enhanced with respect to both the Standard Model and the MSSM.
Sonia El Hedri, Anna Kaminska, Maikel de Vries, Jose Zurita
We perform a general study of the relic density and LHC constraints on simplified models where the dark matter coannihilates with a strongly interacting particle X. In these models, the dark matter depletion is driven by the self-annihilation of X to pairs of quarks and gluons through the strong interaction. The phenomenology of these scenarios therefore only depends on the dark matter mass and the mass splitting between dark matter and X as well as the quantum numbers of X. In this paper, we consider simplified models where X can be either a scalar, a fermion or a vector, as well as a color triplet, sextet or octet. We compute the dark matter relic density constraints taking into account Sommerfeld corrections and bound state formation. Furthermore, we examine the restrictions from thermal equilibrium, the lifetime of X and the current and future LHC bounds on X pair production. All constraints are comprehensively presented in the mass splitting versus dark matter mass plane. While the relic density constraints can lead to upper bounds on the dark matter mass ranging from 2 TeV to more than 10 TeV across our models, the prospective LHC bounds range from 800 to 1500 GeV. A full coverage of the strongly coannihilating dark matter parameter space would therefore require hadron colliders with significantly higher center of mass energies.
Tulika Bose, Antonio Boveia, Caterina Doglioni, Simone Pagan Griso, James Hirschauer, Elliot Lipeles, Zhen Liu, Nausheen R. Shah, Lian-Tao Wang, Kaustubh Agashe, Juliette Alimena, Sebastian Baum, Mohamed Berkat, Kevin Black, Gwen Gardner, Tony Gherghetta, Josh Greaves, Maxx Haehn, Phil C. Harris, Robert Harris, Julie Hogan, Suneth Jayawardana, Abraham Kahn, Jan Kalinowski, Simon Knapen, Ian M. Lewis, Meenakshi Narain, Katherine Pachal, Matthew Reece, Laura Reina, Tania Robens, Alessandro Tricoli, Carlos E. M. Wagner, Riley Xu, Felix Yu, Filip Zarnecki, Amin Aboubrahim, Andreas Albert, Michael Albrow, Wolfgang Altmannshofer, Gerard Andonian, Artur Apresyan, Kétévi Adikle Assamagan, Patrizia Azzi, Howard Baer, Michael J. Baker, Avik Banerjee, Vernon Barger, Brian Batell, Martin Bauer, Hugues Beauchesne, Samuel Bein, Alexander Belyaev, Ankit Beniwal, Mikael Berggren, Prudhvi N. Bhattiprolu, Nikita Blinov, Alain Blondel, Oleg Brandt, Giacomo Cacciapaglia, Rodolfo Capdevilla, Marcela Carena, Cesare Cazzaniga, Francesco Giovanni Celiberto, Cari Cesarotti, Sergei V. Chekanov, Hsin-Chia Cheng, Thomas Y. Chen, Yuze Chen, R. Sekhar Chivukula, Matthew Citron, James Cline, Tim Cohen, Jack H. Collins, Eric Corrigan, Nathaniel Craig, Daniel Craik, Andreas Crivellin, David Curtin, Smita Darmora, Arindam Das, Sridhara Dasu, Annapaola de Cosa, Aldo Deandrea, Antonio Delgado, Zeynep Demiragli, David d'Enterria, Frank F. Deppisch, Radovan Dermisek, Nishita Desai, Abhay Deshpande, Jordy de Vries, Jennet Dickinson, Keith R. Dienes, Karri Folan Di Petrillo, Matthew J. Dolan, Peter Dong, Patrick Draper, Marco Drewes, Etienne Dreyer, Peizhi Du, Florian Eble, Majid Ekhterachian, Motoi Endo, Rouven Essig, Jesse N. Farr, Farida Fassi, Jonathan L. Feng, Gabriele Ferretti, Daniele Filipetto, Thomas Flacke, Karri Folan Di Petrillo, Roberto Franceschini, Diogo Buarque Franzosi, Keisuke Fujii, Benjamin Fuks, Sri Aditya Gadam, Boyu Gao, Aran Garcia-Bellido, Isabel Garcia Garcia, Maria Vittoria Garzelli, Stephen Gedney, Marie-Hélène Genest, Tathagata Ghosh, Mark Golkowski, Giovanni Grilli di Cortona, Emine Gurpinar Guler, Yalcin Guler, C. Guo, Nate Graf, Ulrich Haisch, Jan Hajer, Koichi Hamaguchi, Tao Han, Philip Harris, Sven Heinemeyer, Christopher S. Hill, Joshua Hiltbrand, Tova Ray Holmes, Samuel Homiller, Sungwoo Hong, Walter Hopkins, Shih-Chieh Hsu, Phil Ilten, Wasikul Islam, Sho Iwamoto, Daniel Jeans, Laura Jeanty, Haoyi Jia, Sergo Jindariani, Daniel Johnson, Felix Kahlhoefer, Yonatan Kahn, Paul Karchin, Thomas Katsouleas, Shin-ichi Kawada, Junichiro Kawamura, Chris Kelso, Elham E Khoda, Valery Khoze, Doojin Kim, Teppei Kitahara, Juraj Klaric, Michael Klasen, Kyoungchul Kong, Wojciech Kotlarski, Ashutosh V. Kotwal, Jonathan Kozaczuk, Richard Kriske, Suchita Kulkarni, Jason Kumar, Manuel Kunkel, Greg Landsberg, Kenneth Lane, Clemens Lange, Lawrence Lee, Jiajun Liao, Benjamin Lillard, Lingfeng Li, Shuailong Li, Shu Li, Jenny List, Tong Li, Hongkai Liu, Jia Liu, Jonathan D Long, Enrico Lunghi, Kun-Feng Lyu, Danny Marfatia, Dakotah Martinez, Stephen P. Martin, Navin McGinnis, Karrick McGinty, Krzysztof Mękała, Federico Meloni, Oleksii Mikulenko, Ming Huang, Rashmish K. Mishra, Manimala Mitra, Vasiliki A. Mitsou, Chang-Seong Moon, Alexander Moreno, Takeo Moroi, Gerard Mourou, Malte Mrowietz, Patric Muggli, Jurina Nakajima, Pran Nath, J. Nelson, Matthias Neubert, Laura Nosler, Maria Teresa Núñez Pardo de Vera, Nobuchika Okada, Satomi Okada, Vitalii A. Okorokov, Yasar Onel, Tong Ou, Maksym Ovchynnikov, Rojalin Padhan, Priscilla Pani, Luca Panizzi, Andreas Papaefstathiou, Kevin Pedro, Cristián Peña, Federica Piazza, James Pinfold, Deborah Pinna, Werner Porod, Chris Potter, Markus Tobias Prim, Stefano Profumo, James Proudfoot, Mudit Rai, Filip Rajec, Reese Ramos, Michael J. Ramsey-Musolf, Javier Resta-Lopez, Jürgen Reuter, Andreas Ringwald, Chiara Rizzi, Thomas G. Rizzo, Giancarlo Rossi, Richard Ruiz, L. Rygaard, Aakash A. Sahai, Shadman Salam, Pearl Sandick, Deepak Sathyan, Christiane Scherb, Pedro Schwaller, Leonard Schwarze, Pat Scott, Sezen Sekmen, Dibyashree Sengupta, S. Sen, Anna Sfyrla, Eric Shackelford, T. Sharma, Varun Sharma, Jessie Shelton, William Shepherd, Seodong Shin, Elizabeth H. Simmons, Zoie Sloneker, Carlos Vázquez Sierra, Torbjörn Sjöstrand, Scott Snyder, Huayang Song, Giordon Stark, Patrick Stengel, Joachim Stohr, Daniel Stolarski, Matt Strassler, Nadja Strobbe, Julia Gonski, Rebeca Gonzalez Suarez, Taikan Suehara, Shufang Su, Wei Su, Raza M. Syed, Tim M. P. Tait, Toshiki Tajima, Andy Tang, Xerxes Tata, Teodor Tchalokov, Andrea Thamm, Brooks Thomas, Natalia Toro, Nhan V. Tran, Loan Truong, Yu-Dai Tsai, Eva Tuecke, Nikhilesh Venkatasubramanian, Chris B. Verhaaren, Carl Vuosalo, Xiao-Ping Wang, Xing Wang, Yikun Wang, Zhen Wang, Christian Weber, Glen White, Martin White, Anthony G. Williams, Brady Williams, Mike Williams, Stephane Willocq, Alex Woodcock, Yongcheng Wu, Ke-Pan Xie, Keping Xie, Si Xie, C. -H. Yeh, Ryo Yonamine, David Yu, S. -S. Yu, Mohamed Zaazoua, Aleksander Filip Żarnecki, Kamil Zembaczynski, Danyi Zhang, Jinlong Zhang, Frank Zimmermann, Jose Zurita
Carlotta Accettura, Dean Adams, Rohit Agarwal, Claudia Ahdida, Chiara Aimè, Nicola Amapane, David Amorim, Paolo Andreetto, Fabio Anulli, Robert Appleby, Artur Apresyan, Aram Apyan, Sergey Arsenyev, Pouya Asadi, Mohammed Attia Mahmoud, Aleksandr Azatov, John Back, Lorenzo Balconi, Laura Bandiera, Roger Barlow, Nazar Bartosik, Emanuela Barzi, Fabian Batsch, Matteo Bauce, J. Scott Berg, Andrea Bersani, Alessandro Bertarelli, Alessandro Bertolin, Fulvio Boattini, Alex Bogacz, Maurizio Bonesini, Bernardo Bordini, Salvatore Bottaro, Luca Bottura, Alessandro Braghieri, Marco Breschi, Natalie Bruhwiler, Xavier Buffat, Laura Buonincontri, Philip Burrows, Graeme Burt, Dario Buttazzo, Barbara Caiffi, Marco Calviani, Simone Calzaferri, Daniele Calzolari, Rodolfo Capdevilla, Christian Carli, Fausto Casaburo, Massimo Casarsa, Luca Castelli, Maria Gabriella Catanesi, Gianluca Cavoto, Francesco Giovanni Celiberto, Luigi Celona, Alessandro Cerri, Gianmario Cesarini, Cari Cesarotti, Grigorios Chachamis, Antoine Chance, Siyu Chen, Yang-Ting Chien, Mauro Chiesa, Anna Colaleo, Francesco Collamati, Gianmaria Collazuol, Marco Costa, Nathaniel Craig, Camilla Curatolo, David Curtin, Giacomo Da Molin, Magnus Dam, Heiko Damerau, Sridhara Dasu, Jorge de Blas, Stefania De Curtis, Ernesto De Matteis, Stefania De Rosa, Jean-Pierre Delahaye, Dmitri Denisov, Haluk Denizli, Christopher Densham, Radovan Dermisek, Luca Di Luzio, Elisa Di Meco, Biagio Di Micco, Keith Dienes, Eleonora Diociaiuti, Tommaso Dorigo, Alexey Dudarev, Robert Edgecock, Filippo Errico, Marco Fabbrichesi, Stefania Farinon, Anna Ferrari, Jose Antonio Ferreira Somoza, Frank Filthaut, Davide Fiorina, Elena Fol, Matthew Forslund, Roberto Franceschini, Rui Franqueira Ximenes, Emidio Gabrielli, Michele Gallinaro, Francesco Garosi, Luca Giambastiani, Alessio Gianelle, Simone Gilardoni, Dario Augusto Giove, Carlo Giraldin, Alfredo Glioti, Mario Greco, Admir Greljo, Ramona Groeber, Christophe Grojean, Alexej Grudiev, Jiayin Gu, Chengcheng Han, Tao Han, John Hauptman, Brian Henning, Keith Hermanek, Matthew Herndon, Tova Ray Holmes, Samuel Homiller, Guoyuan Huang, Sudip Jana, Sergo Jindariani, Yonatan Kahn, Ivan Karpov, David Kelliher, Wolfgang Kilian, Antti Kolehmainen, Kyoungchul Kong, Patrick Koppenburg, Nils Kreher, Georgios Krintiras, Karol Krizka, Gordan Krnjaic, Nilanjana Kumar, Anton Lechner, Lawrence Lee, Qiang Li, Roberto Li Voti, Ronald Lipton, Zhen Liu, Shivani Lomte, Kenneth Long, Jose Lorenzo Gomez, Roberto Losito, Ian Low, Qianshu Lu, Donatella Lucchesi, Lianliang Ma, Yang Ma, Shinji Machida, Fabio Maltoni, Marco Mandurrino, Bruno Mansoulie, Luca Mantani, Claude Marchand, Samuele Mariotto, Stewart Martin-Haugh, David Marzocca, Paola Mastrapasqua, Giorgio Mauro, Andrea Mazzolari, Navin McGinnis, Patrick Meade, Barbara Mele, Federico Meloni, Matthias Mentink, Claudia Merlassino, Elias Metral, Rebecca Miceli, Natalia Milas, Nikolai Mokhov, Alessandro Montella, Tim Mulder, Riccardo Musenich, Marco Nardecchia, Federico Nardi, Niko Neufeld, David Neuffer, Yasar Onel, Domizia Orestano, Daniele Paesani, Simone Pagan Griso, Mark Palmer, Paolo Panci, Giuliano Panico, Rocco Paparella, Paride Paradisi, Antonio Passeri, Nadia Pastrone, Antonello Pellecchia, Fulvio Piccinini, Alfredo Portone, Karolos Potamianos, Marco Prioli, Lionel Quettier, Emilio Radicioni, Raffaella Radogna, Riccardo Rattazzi, Diego Redigolo, Laura Reina, Elodie Resseguie, Jürgen Reuter, Pier Luigi Ribani, Cristina Riccardi, Lorenzo Ricci, Stefania Ricciardi, Luciano Ristori, Tania Natalie Robens, Werner Rodejohann, Chris Rogers, Marco Romagnoni, Kevin Ronald, Lucio Rossi, Richard Ruiz, Farinaldo S. Queiroz, Filippo Sala, Paola Sala, Jakub Salko, Paola Salvini, Ennio Salvioni, Jose Santiago, Ivano Sarra, Francisco Javier Saura Esteban, Jochen Schieck, Daniel Schulte, Michele Selvaggi, Carmine Senatore, Abdulkadir Senol, Daniele Sertore, Lorenzo Sestini, Varun Sharma, Vladimir Shiltsev, Jing Shu, Federica Maria Simone, Rosa Simoniello, Kyriacos Skoufaris, Massimo Sorbi, Stefano Sorti, Anna Stamerra, Steinar Stapnes, Giordon Holtsberg Stark, Marco Statera, Bernd Stechauner, Daniel Stolarski, Diktys Stratakis, Shufang Su, Wei Su, Olcyr Sumensari, Xiaohu Sun, Raman Sundrum, Maximilian J Swiatlowski, Alexei Sytov, Benjamin T. Kuchma, Tim M. P. Tait, Jian Tang, Jingyu Tang, Andrea Tesi, Pietro Testoni, Brooks Thomas, Emily Anne Thompson, Riccardo Torre, Ludovico Tortora, Luca Tortora, Sokratis Trifinopoulos, Ilaria Vai, Riccardo Valente, Riccardo Umberto Valente, Marco Valente, Alessandro Valenti, Nicolò Valle, Ursula van Rienen, Rosamaria Venditti, Arjan Verweij, Piet Verwilligen, Ludovico Vittorio, Paolo Vitulo, Liantao Wang, Hannsjorg Weber, Mariusz Wozniak, Richard Wu, Yongcheng Wu, Andrea Wulzer, Keping Xie, Akira Yamamoto, Yifeng Yang, Katsuya Yonehara, Angela Zaza, Xiaoran Zhao, Alexander Zlobin, Davide Zuliani, Jose Zurita
Juliette Alimena, James Beacham, Martino Borsato, Yangyang Cheng, Xabier Cid Vidal, Giovanna Cottin, Albert De Roeck, Nishita Desai, David Curtin, Jared A. Evans, Simon Knapen, Sabine Kraml, Andre Lessa, Zhen Liu, Sascha Mehlhase, Michael J. Ramsey-Musolf, Heather Russell, Jessie Shelton, Brian Shuve, Monica Verducci, Jose Zurita, Todd Adams, Michael Adersberger, Cristiano Alpigiani, Artur Apresyan, Robert John Bainbridge, Varvara Batozskaya, Hugues Beauchesne, Lisa Benato, S. Berlendis, Eshwen Bhal, Freya Blekman, Christina Borovilou, Jamie Boyd, Benjamin P. Brau, Lene Bryngemark, Oliver Buchmueller, Malte Buschmann, William Buttinger, Mario Campanelli, Cari Cesarotti, Chunhui Chen, Hsin-Chia Cheng, Sanha Cheong, Matthew Citron, Andrea Coccaro, V. Coco, Eric Conte, Félix Cormier, Louie D. Corpe, Nathaniel Craig, Yanou Cui, Elena Dall'Occo, C. Dallapiccola, M. R. Darwish, Alessandro Davoli, Annapaola de Cosa, Andrea De Simone, Luigi Delle Rose, Frank F. Deppisch, Biplab Dey, Miriam D. Diamond, Keith R. Dienes, Sven Dildick, Babette Döbrich, Marco Drewes, Melanie Eich, M. ElSawy, Alberto Escalante del Valle, Gabriel Facini, Marco Farina, Jonathan L. Feng, Oliver Fischer, H. U. Flaecher, Patrick Foldenauer, Marat Freytsis, Benjamin Fuks, Iftah Galon, Yuri Gershtein, Stefano Giagu, Andrea Giammanco, Vladimir V. Gligorov, Tobias Golling, Sergio Grancagnolo, Giuliano Gustavino, Andrew Haas, Kristian Hahn, Jan Hajer, Ahmed Hammad, Lukas Heinrich, Jan Heisig, J. C. Helo, Gavin Hesketh, Christopher S. Hill, Martin Hirsch, M. Hohlmann, W. Hulsbergen, John Huth, Philip Ilten, Thomas Jacques, Bodhitha Jayatilaka, Geng-Yuan Jeng, K. A. Johns, Toshiaki Kaji, Gregor Kasieczka, Yevgeny Kats, Malgorzata Kazana, Henning Keller, Maxim Yu. Khlopov, Felix Kling, Ted R. Kolberg, Igor Kostiuk, Emma Sian Kuwertz, Audrey Kvam, Greg Landsberg, Gaia Lanfranchi, Iñaki Lara, Alexander Ledovskoy, Dylan Linthorne, Jia Liu, Iacopo Longarini, Steven Lowette, Henry Lubatti, Margaret Lutz, Jingyu Luo, Judita Mamužić, Matthieu Marinangeli, Alberto Mariotti, Daniel Marlow, Matthew McCullough, Kevin McDermott, P. Mermod, David Milstead, Vasiliki A. Mitsou, Javier Montejo Berlingen, Filip Moortgat, Alessandro Morandini, Alice Polyxeni Morris, David Michael Morse, Stephen Mrenna, Benjamin Nachman, Miha Nemevšek, Fabrizio Nesti, Christian Ohm, Silvia Pascoli, Kevin Pedro, Cristián Peña, Karla Josefina Pena Rodriguez, Jónatan Piedra, James L. Pinfold, Antonio Policicchio, Goran Popara, Jessica Prisciandaro, Mason Proffitt, Giorgia Rauco, Federico Redi, Matthew Reece, Allison Reinsvold Hall, H. Rejeb Sfar, Sophie Renner, Amber Roepe, Manfredi Ronzani, Ennio Salvioni, Arka Santra, Ryu Sawada, Jakub Scholtz, Philip Schuster, Pedro Schwaller, Cristiano Sebastiani, Sezen Sekmen, Michele Selvaggi, Weinan Si, Livia Soffi, Daniel Stolarski, David Stuart, John Stupak, Kevin Sung, Wendy Taylor, Sebastian Templ, Brooks Thomas, Emma Torró-Pastor, Daniele Trocino, Sebastian Trojanowski, Marco Trovato, Yuhsin Tsai, C. G. Tully, Tamás Álmos Vámi, Juan Carlos Vasquez, Carlos Vázquez Sierra, K. Vellidis, Basile Vermassen, Martina Vit, Devin G. E. Walker, Xiao-Ping Wang, Gordon Watts, Si Xie, Melissa Yexley, Charles Young, Jiang-Hao Yu, Piotr Zalewski, Yongchao Zhang
Cristiano Alpigiani, Austin Ball, Liron Barak, James Beacham, Yan Benhammo, Tingting Cao, Paolo Camarri, Roberto Cardarelli, Mario Rodriguez-Cahuantzi, John Paul Chou, David Curtin, Miriam Diamond, Giuseppe Di Sciascio, Marco Drewes, Sarah C. Eno, Erez Etzion, Rouven Essig, Jared Evans, Oliver Fischer, Stefano Giagu, Brandon Gomes, Andy Haas, Yuekun Heng, Giuseppe Iaselli, Ken Johns, Muge Karagoz, Luke Kasper, Audrey Kvam, Dragoslav Lazic, Liang Li, Barbara Liberti, Zhen Liu, Henry Lubatti, Giovanni Marsella, Matthew McCullough, David McKeen, Patrick Meade, Gilad Mizrachi, David Morrissey, Meny Raviv Moshe, Karen Salome Caballero-Mora, Piter A. Paye Mamani, Antonio Policicchio, Mason Proffitt, Marina Reggiani-Guzzo, Joe Rothberg, Rinaldo Santonico, Marco Schioppa, Jessie Shelton, Brian Shuve, Martin A. Subieta Vasquez, Daniel Stolarski, Albert de Roeck, Arturo Fernandez Tellez, Guillermo Tejeda Munoz, Mario Ivan Martinez Hernandez, Yiftah Silver, Steffie Ann Thayil, Emma Torro, Yuhsin Tsai, Juan Carlos Arteaga-Velazquez, Gordon Watts, Charles Young, Jose Zurita
In this Letter of Intent (LOI) we propose the construction of MATHUSLA (MAssive Timing Hodoscope for Ultra-Stable neutraL pArticles), a dedicated large-volume displaced vertex detector for the HL-LHC on the surface above ATLAS or CMS. Such a detector, which can be built using existing technologies with a reasonable budget in time for the HL-LHC upgrade, could search for neutral long-lived particles (LLPs) with up to several orders of magnitude better sensitivity than ATLAS or CMS, while also acting as a cutting-edge cosmic ray telescope at CERN to explore many open questions in cosmic ray and astro-particle physics. We review the physics motivations for MATHUSLA and summarize its LLP reach for several different possible detector geometries, as well as outline the cosmic ray physics program. We present several updated background studies for MATHUSLA, which help inform a first detector-design concept utilizing modular construction with Resistive Plate Chambers (RPCs) as the primary tracking technology. We present first efficiency and reconstruction studies to verify the viability of this design concept, and we explore some aspects of its total cost. We end with a summary of recent progress made on the MATHUSLA test stand, a small-scale demonstrator experiment currently taking data at CERN Point 1, and finish with a short comment on future work.
Kingman Cheung, Oliver Fischer, Zeren Simon Wang, Jose Zurita
Profiling the Higgs boson requires the study of its non-standard decay modes. In this work we discuss the prospects of the Large Hadron electron Collider (LHeC) to detect scalar particles with masses $\gtrsim$ 10 GeV produced from decays of the Standard Model (SM) Higgs boson. These scalar particles decay mainly to bottom pairs, and in a vast portion of the allowed parameter space they acquire a macroscopic lifetime, hence giving rise to displaced hadronic vertices. The LHeC provides a very clean environment that allows for easy identification of these final states, in contrast to hadronic colliders where the overwhelming backgrounds and high pile-up render such searches incredibly challenging. We find that the LHeC provides a unique window of opportunity to detect scalar particles with masses between 10 GeV and half the SM Higgs mass. In the Higgs Portal scenarios we can test the mixing angle squared, $\sin^2 α$, as low as $10^{-5} - 10^{-7}$, with the exact value depending on the vacuum expectation value of the new scalar. Our results are also presented in a model-independent fashion in the lifetime-branching ratio and mass-branching ratio planes. We have found that exotic branching ratios of the Higgs boson at the sub-percent level can be probed, for the scalar decay length in the range $10^{-4}$ m $\lesssim c τ\lesssim 10^{-1}$ m. The expected coverage of the parameter space largely exceeds the published sensitivity of the indirect reach at the high-luminosity Large Hadron Collider via the invisible Higgs branching ratio.
Martino Borsato, Xabier Cid Vidal, Yuhsin Tsai, Carlos Vázquez Sierra, José Zurita, Gonzalo Alonso-Álvarez, Alexey Boyarsky, Alexandre Brea Rodríguez, Diogo Buarque Franzosi, Giacomo Cacciapaglia, Adrián Casais Vidal, Mingxuan Du, Gilly Elor, Miguel Escudero, Gabriele Ferretti, Thomas Flacke, Patrick Foldenauer, Jan Hajer, Louis Henry, Philip Ilten, Jernej Kamenik, Brij Kishor Jashal, Simon Knapen, Federico Leo Redi, Matthew Low, Zuowei Liu, Arantza Oyanguren Campos, Erica Polycarpo, Maria Ramos, Miguel Ramos Pernas, Ennio Salvioni, Murilo Santana Rangel, Ruth Schäfer, Lorenzo Sestini, Yotam Soreq, Van Que Tran, Inar Timiryasov, Maarten van Veghel, Susanne Westhoff, Michael Williams, Jure Zupan
In this paper, we describe the potential of the LHCb experiment to detect Stealth physics. This refers to dynamics beyond the Standard Model that would elude searches that focus on energetic objects or precision measurements of known processes. Stealth signatures include long-lived particles and light resonances that are produced very rarely or together with overwhelming backgrounds. We will discuss why LHCb is equipped to discover this kind of physics at the Large Hadron Collider and provide examples of well-motivated theoretical models that can be probed with great detail at the experiment.
Daniel de Florian, Jose Zurita
We present the first calculation of two-quark and five-gluon tree amplitudes using on-shell recursion relations. These amplitudes are needed for tree level 5-jet cross-section and an essential ingredient for next-to-leading order 4-jet and next-to-next-to-leading order 3-jet production at hadronic colliders. Very compact expressions for all possible helicity configurations are provided, allowing for direct implementation in Monte-Carlo codes.
Juliana Carrasco, José Zurita
A strongly interacting dark sector can give rise to a class of signatures dubbed dark showers, where in analogy to the strong sector in the Standard Model, the dark sector undergoes its own showering and hadronization, before decaying into Standard Model final states. When the typical decay lengths of the dark sector mesons are larger than a few centimeters (and no larger than a few meters) they give rise to the striking signature of emerging jets, characterized by a large multiplicity of displaced vertices. In this article we consider the general reinterpretation of the CMS search for emerging jets plus prompt jets into arbitrary new physics scenarios giving rise to emerging jets. More concretely, we consider the cases where the SM Higgs mediates between the dark sector and the SM, for several benchmark decay scenarios. Our procedure is validated employing the same model than the CMS emerging jet search. We find that emerging jets can be the leading probe in regions of parameter space, in particular when considering the so-called gluon-portal and dark photon-portal decay benchmarks. With the current 16.1 fb$^{-1}$ of luminosity this search can exclude down to ${\cal O} (20) \% $ exotic branching ratio of the SM Higgs, but a naive extrapolation to the 139 fb$^{-1}$ luminosity employed in the current model-independent, indirect bound of 16% would probe exotic branching ratios into dark quarks down to below 10%. Further extrapolating these results to the HL-LHC, we find that one can pin down exotic branching ratio values of 1%, which is below the HL-LHC expectations of 2.5$-$4%. We make our recasting code publicly available, as part of the LLP Recasting Repository.
Florian Goertz, Andreas Papaefstathiou, Li Lin Yang, José Zurita
We derive the constraints that can be imposed on the dimension-6 effective theory extension of the Standard Model, using gluon fusion-initiated Higgs boson pair production at the LHC. We use a realistic analysis focussing on the $hh \rightarrow (b\bar{b}) ( τ^+ τ^- )$ final state, including initial-state radiation and non-perturbative effects. We include the statistical uncertainties on the signal rates as well as conservative estimates of the theoretical uncertainties. We first consider a theory containing only modifications of the trilinear coupling, through a $c_6 λ\, H^6/ v^2$ Lagrangian term, and then examine the full parameter space of the effective theory, incorporating current bounds obtained through single Higgs boson measurements. We also consider an alternative scenario, where we vary a smaller sub-set of parameters. Allowing, finally, the values of the other coefficients to vary within \textit{projected} experimental ranges, we find that the currently unbounded parameter, $c_6$, could be constrained to lie within $|c_6| \lesssim 0.6$ at 1$σ$ confidence, at the end of the high-luminosity run of the LHC (14~TeV) in the full model, and to $-0.6 \lesssim c_6 \lesssim 0.5$ in the alternative model. This study constitutes a first step towards the inclusion of multi-Higgs boson production in a full fit to the dimension-6 effective field theory framework.