Test of lepton universality using B0→KS0l+l- and B+→K*+l+l- decays.
Today at the CERN seminar and at the Rencontres de Blois the LHCb Collaboration presented new tests of lepton universality, one of the basic principles of the Standard Model (SM) of particle physics. This principle states that the SM treats the three charged leptons (electrons, muons and taus) identically, except for differences due to their different masses. The new measurements, while of limited statistical sensitivity, exhibit the same coherent pattern of deviations from lepton universality as seen in previous LHCb results.
In March 2021, the collaboration reported an evidence at 3.1 standard deviations (σ) for the breaking of lepton universality in a measurement of the ratio RK. The ratio RK describes how often a B+ meson decays to a charged kaon and either a positive and a negatively charge muon (K+μ+μ-) or a positron-electron pair (K+e+e-). These decays are extremely rare, occurring at a rate of only one in two million B+ meson decays. The decays involve the transformation of a beauty quark into a strange quark (b→s), a process that is highly suppressed in the Standard Model and can be affected by the existence of new particles, which could have masses too high to be produced directly at the Large Hadron Collider. The left graph shows Standard Model contributions involving γ, W+, and Z0 bosons. The right one shows a possible new physics contribution to the decay with a hypothetical leptoquark (LQ) which, unlike the Standard Model bosons, could have different interaction strengths with the different types of leptons.
Deviations at the level of 2.2-2.5 σ in a measurement of the ratio RK*0 were also reported in April 2017.
Both ratios exhibit a deficit of μ+μ- pairs with respect to e+e- pairs. Today’s results also report tests of lepton universality, using ratios RK and RK*. However, in this measurement, K and K* mesons with different electric charges have been used. Physicists call these newly measured decays the“isospin partners” of the previously measured decays. The new ratios are labelled RKS0 and RK*+.
LHCb has studied a number of other such ratios comparing decays with different leptons (l=e, μ, or τ leptons) in beauty particle decays (see R(D*), R(J/ψ) and R(pK)). These results revealed hints of deviations from lepton universality, none of which is significant enough to constitute an observation of new physics on its own. However, according to theorists who study possible extensions of the SM, these deviations combined suggest an interesting and coherent pattern, which could be evidence for physics beyond the SM.
The values of the RKS0 and RK*+ ratios are presented at the top of this article. These ratios correspond to the transitions B0→KS0l+l- and B+→K*+l+l-.
Figure 1. Quark diagrams for a B0→KS0l+l- decay.
The ratios are also presented in figure 2 for different regions of the dilepton invariant mass squared, q2. They are individually consistent with the SM at the 1.4 and 1.5σ level, their combination at the 2σ level (for experts: using a fit for a single Wilson coefficient). It is interesting to note that the central values exhibit the same coherent pattern of deviation as the other lepton universality tests performed by LHCb – the muon pairs are observed less frequently than the electron pairs. The image to the left lists the new measurements by LHCb, the most precise to date, of RKS0 and RK*+ ratios, and previous measurments by Belle.

Figure 2. RKS0 and RK*+ Ratios for different regions of the dilepton invariant mass squared, q2
The bottom left image above shows the KS0μ+μ- mass distribution and the bottom right image the KS0e+e- mass used to determine the RKS0 ratio. The top left image shows the KS0π+ μ+μ- mass distribution and the top right the KS0π+e+e- mass distribution used to determine the RK*+ ratio. Note that a K*+ meson decays into a KS0 and a π+ meson and note also a clear accumulation of events at the B0 or B+ mass.
The Institute of Cosmos Sciences of the University of Barcelona participates in this experiment with the researchers Carla Marín, Eugeni Graugés, Lluís Garrido, Ricardo Vázquez who have contributed to the development and optimisation of the electron reconstruction process, which is a crucial ingredient in the obtention of these measurements. We should also mention that the ICC-LHCb group counts with a new addition to their team, PhD Student Albert López, who will work on a similar Lepton Universality measurements as described in this news item with baryons. He will analyse the transition Λb0→pK-l+l-
Read more in the LHCb presentations at CERN and at Blois, and in the LHCb paper. You can also stay on the loop of the announcements of new results by following the experiment’s twitter account @LHCbExperiment.
The ICCUB postdoctoral researcher Ryotaku Suzuki has been recognized by the XVI edition of the prestigious Seitaro Nakamura award for his work on the paper “Topology-changing horizons at large D as Ricci flows" which was published in 2019 alongside ICCUB’s senior researcher Roberto Emparan as co-author.
Dr. Suzuki joined the Institute of Cosmos Sciences of the University of Barcelona in 2018 as a member of the gravitation and cosmology research group and has since worked in several areas including general relativity in the large D limit.
The award, which is named after Dr. Seitaro Nakamura (1913-2007) who had produced substantial research on theoretical particle physics particularly on two-meson and beta decay, was established in 2006 in order to encourage young researchers for their future endeavors in theoretical physics and the related fields.
This distinction is bestowed upon researchers between the ages of 35 and 40 who have remarkable scientific production levels. The grant consists of 40.000€ that will support the realization of Antoja's research project "Analysis of the shake that our Galaxy suffered in the recent past" in the field of Galaxy formation and evolution.
The award is not only given to scientific areas but also to cultural creators in fields of art or technology thus becoming a transversal support motor.
You can read more about this on the following link.
The ceremony took place last Tuesday, June 8, in the Palau de la Generalitat and it was chaired by the President of the Comunitat Valenciana Ximo Puig.
Licia Verde joined the ICCUB as an ICREA researcher on 2009. She has carried her research in several fields in all of which she has become a key referent: from theoretical Cosmology and Cosmic Microwave radiation to Large Scale Structure, Galaxy Clusters or Statistical Applications to precision Cosmology. Throughout her career, she has been involved in the main cosmology projects such as 2dF Galaxy Redshift Survey (2dFGRS), Wilkinson Microwave Anisotropy Probe (WMAP), Sloan Digital Sky Survey (SDSS) and the Dark Energy Spectroscopic Instrument (DESI).
She stands on a long list of awards and distinctions: the Gruber Prize for Cosmology (2012), the Group Achievement NASA award (for her contribution on the Wilkinson Microwave Anisotropy Probe space mission, the National Research Award of the Generalitat de Catalunya (2018) and the Narcís Monturiol Medal (2019), all of which are a testimony to her scientific career.
You can learn more about her research in the piece: «Licia Verde: una carrera reconeguda en cosmologia de precisió»
The master's degree in Quantum Science and Technologies, coordinated by the University of Barcelona, is the result of common effort of the University of Barcelona, the Autonomous University of Barcelona, the Polytechnic University of Catalonia, the Institute of Photonic Sciences, the Barcelona Supercomputing Center, the Institute of High Energy Physics and the Catalan Institute of Nanoscience and Nanotechnology. It arises in parallel to the establishment of the emerging community in Quantum Technologies, QuantumCat.
The program is aimed at graduates in Physics, Physical Engineering or equivalent degrees who want to continue specialization studies in Quantum Science and Technologies and its fundamental objectives are on the one hand to provide a solid education in theoretical physics and quantum information theory and to offer a variety of elective subjects to form a forward-looking study plan oriented to the development of quantum science and technology.
The program is taught by 30+ expert professors, and covers the core concepts of quantum science and technology, as well as practical tools and techniques.
The master gives access to cutting-edge theoretical and experimental research in the fields of quantum sensing, communication, computing and simulation.
Direct connections to industry through the QuantumCAT community, and the participation of high-tech companies in the teaching program and an annual careers symposium, will facilitate the future integration of students in both academic and industrial sectors.
Prof Bruno Julia, member of the Institute of Cosmos Sciences and coordinator of the Master in the Quantum Science and Technology program notes, “Quantum physics will play a major role in the next future developments in our capacity to compute, communicate, and measure with precision. A solid education in Quantum sciences will be a crucial asset to both push the boundaries of our knowledge and also to develop new industrial products profiting from the intricate quantum properties. This master is the seed for a quantum future.”
Prof. Morgan Mitchell, Coordinator QuantumCAT, the Quantum Technologies Hub of Catalonia, adds, “Quantum technology is growing rapidly in Catalonia, with universities, research centres, startup companies and established industrials all working to bring about the second quantum revolution. QuantumCAT, strongly supports the creation of the Master in QST, as a way to boost the skilled workforce in this dynamic industry. We look forward to working with MQST students and graduates.”
The Spanish Royal Physics Society has announced today the “Real Sociedad Española de Física - Fundación BBVA 2020” Physics Prizes. Dr. Héctor Gil-Marín, a researcher in cosmology at the Institute of Cosmos Sciences (ICCUB) and a postdoctoral Junior Leader “la Caixa” fellow, has been rewarded with the Young Researcher Award in Theoretical Physics.
The jury highlights his outstanding contributions to the analysis and interpretation of galaxy mapping, advancing our understanding of the accelerated Universe, being undoubtedly one of the most brilliant researchers in the field of the cosmology of his generation.
Dr. Gil-Marín was a member of the BOSS and eBOSS international collaborations and is a current researcher of DESI, where he plays a leading role in the survey mapping. He actively participated in the analysis of BOSS and eBOSS data, which resulted in the recently published largest three-dimensional map of the distribution of galaxies. His research is focused on the large-scale structure of the Universe, and he intends to answer one of the most fundamental questions in cosmology for the past 20 years, what drives the late-time accelerated expansion of the Universe.
Dr. Héctor Gil-Marín biography
Dr. Héctor Gil-Marín obtained a PhD in Physics in 2012 at the Universitat de Barcelona. Prof. Gil-Marín has been a postdoctoral research associate at the Institute of Cosmology and Gravitation, University of Portsmouth (UK) and a Lagrange fellow at the LPNHE at the Université Pierre et Marie Curie (Paris). From 2018 Dr. Gil-Marin holds a Junior Leader 'La Caixa' fellowship at the ICCUB.
Selected publications
The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of the structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0 Arxiv
Blind Observers of the Sky. Arxiv
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: BAO measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies. Arxiv
The power spectrum and bispectrum of SDSS DR11 BOSS galaxies - I. Bias and gravity. Arxiv
More information:
- Website
- ORCID
Read the full article at Astronomy & Astrophysics
The thesis "Radiación no térmica asociada a estrellas de gran massa", defended by Dr. Santiago del Palacio in 2018 under the direction of the researcher of the Institute of Cosmos Sciences, Prof. Valentí Bosch-Ramón, has been selected by the jury appointed by the Associació Argentina de Astronomía, the organizing body.
The Carlos M. Varsavsky Prize for the best doctoral thesis has a biennial character and has been awarded since 2006. Its aim is to promote and recognize scientific research and academic activity in Argentine astronomy and astrophysics.
The jury highlights the impact that the thesis has had in its area of ??research with the publication of articles in international journals and scientific meetings. In the thesis of Dr. del Palacio is investigated the nonthermal emission produced in systems with stars of great mass. The aim is to understand the acceleration efficiency of cosmic rays in these systems, under what conditions they are capable of being non-thermal emitters and what are the characteristics of their magnetic fields, managing to combine the observation and theory behind the issuance of these objects.
The Spanish Ministry of Science and Innovation has published the resolution of the 2019 call, where the Institute of Cosmos Sciences is one of the six Maria de Maeztu Excellence Units that is accredited this year. This is the second time that our Institute receives this award, after the first one obtained in the 2014 competitive call.
This recognition distinguishes organizations with highly competitive research programs that are among the best in the world in their respective scientific areas. The evaluation and selection process is carried out independently by an international scientific committee of widely recognized researchers, which selects both Severo Ochoa centers and Maria de Maeztu units under the same requirements and criteria. The ICCUB is one of the 16 organizations (10 Severo Ochoa centers and 6 Maria de Maeztu units) that has been selected in this annual competitive call, among 55 candidates.
The accreditation provides funding to research organizations that demonstrate international scientific impact and leadership, and actively embrace knowledge transfer and collaboration with the business sector. Efforts on scientific publications access researcher’s effort with open access policies to scientific publications, outreach and knowledge diffusion are also recognized.
The Maria de Maeztu recognition is valid for four years, and provides 500.000€ each year. This strengthens research initiatives and helps attract and grow the research community.
As a Unit of Excellence, our Institute will join the SOMM Excellence Alliance, which promotes Spanish Excellence in research and enhances its social impact at national and international levels.
The Institute of Cosmos Sciences
The Institute of Cosmos Sciences (ICCUB, http://icc.ub.edu) is a research institute of the University of Barcelona (UB). It is an interdisciplinary center dedicated to fundamental research in the fields of cosmology, astrophysics, and particle physics. In addition, the institute has a strong technology program through its participation in international collaborations in observational astronomy and experimental particle physics. Created in 2006, the ICCUB brought together professors and researchers who worked in various departments at the UB Faculty of Physics. Our research lines are motivated by three main questions:
1. What are the origin and fate of the Universe?
2. What are the constituents of the Universe?
3. Why does the Universe have its current appearance?
The search for answers inspires the institute to define and review its research priorities towards scientific and technological advances. At the same time, the institute focuses on the new opportunities offered by technological developments related to its research areas, in order to revert them to society. Moreover, the ICCUB participates in many key international scientific consortia and projects, such as the Large Hadron Collider, the Gaia astrometric space mission, the MAGIC / CTA high-energy astrophysics telescopes, and the Virgo gravitational wave detector, among others.
The ICCUB is located on the north campus of the University of Barcelona, in the facilities of the Faculty of Physics, and at the Barcelona Science Park. It is also one of the four units that constitute the Institute for Space Studies of Catalonia (http://www.ieec.cat/es/).
Awarded Severo Ochoa Centers and Maria de Maeztu units
Eight Severo Ochoa centers have renewed their accreditation: Centro Nacional de Investigaciones Oncológicas (CNIO), Instituto de Ciencias Matemáticas (ICMAT), Instituto de Ciencias Fotónicas (ICFO), Instituto de Investigación Biomédica, Barcelona Graduate School of Economics (BGSE), Instituto de Astrofísica de Canarias (IAC), Centro de Investigación Agrigenómica (CRAG), and the Instituto de Ciencia de Materiales de Barcelona (ICMAB). In addition the Instituto Catalán de Investigación Química (ICIQ) recovers this distinction, which was first received in 2013.
Our Institute has recovered the Maria de Maeztu distinction, received first in 2014. Two units have renewed their distinction as units of excellence María de Maeztu: the Instituto de Ciencia Molecular of the Universidad de Valencia (ICMol), the Instituto de Tecnología y Ciencia Ambientales (ITCA), of the Universidad Autónoma de Barcelona. In addition, three institutions have received the distinction for the first time: the Instituto Imdea Energía, the Departamento de Agronomía de la Universidad de Córdoba, and the Instituto Catalán de Paleoncología Humana y Evolución Social.
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