Conférences  >  Physique  >  Astronomie, astrophysique et cosmologie

Yukawa Institute for Theoretical Physics, Kyoto University

Cours et événements pour étudiants en physique,    Mécanique quantique et technologie quantique

Isaac Newton Institute for Mathematical Sciences (INI)

Defining a theory of quantum gravity remains one of the most challenging problems at the cutting edge of research in mathematical and theoretical physics. Unlocking this problem implies constructing a quantum field theoretic description of gravity which fully elucidates how a quantum field theory encodes gravitational spacetime background solutions. Much of the progress in shaping the language and the framework of this problem owes its genesis to a specific subset of problems in quantum gravity, namely those dealing with understanding the organisation of information in black holes.

Isaac Newton Institute for Mathematical Sciences (INI)

This workshop aims to bring together researchers from number theory, automorphic representation theory and string theory to explore how automorphic forms that encode degeneracies of BPS could be related to and feed into information theoretic concepts such as quantum error corrections, applied to BPS and near-extremal black hole backgrounds, and to develop machine learning techniques to unveil some of the hitherto undefined automorphic structures underlying the generating functions for BPS black hole microstates in superstring models. This event is the first workshop of the 4-month long BLH programme at the INI centred around the same topics.

Réseaux de neurones et intelligence artificielle, apprentissage automatique,    Théorie des nombres, arithmétique

Alikhanian National Laboratory (Yerevan Physics Institute), Armenia

This is a Conference on Particle Physics and Cosmology dedicated to memory of Valery Rubakov who passed away in October 2022. The idea is to get together people from over the world to discuss the domains of physics he worked in and made breakthrough contributions.

particle physics, cosmology, HEP, QCD, Neutrino Physics, Gravity, astroparticle physics

The Arnold Sommerfeld Center for Theoretical Physics at the LMU in Munich will host a school on “The Quantum Gravity Swampland and its consequences for the observable world” in the period October 9-13, 2023. We plan to have the school in presence, in accordance with the Corona rules then in force. The school is primarily aimed at PhD students, but master students or more senior researchers are very welcome to apply as well. It will cover introductory lectures to the swampland program as well as more advanced topics on formal developments and phenomenological applications to particle physics and cosmology.

Physique des hautes énergies, des particules et des champs,    Cours et événements pour étudiants en physique

Email.: https://www.munich-iapbp.de/magnetic-fields

Institute for Astrophysics of Andalucia / University of Málaga

14 years after the celebration of the First Workshop on robotic autonomous observatories in Málaga, the number of automatic astronomical facilities worldwide has significantly grown, as well as the level of robotisation, autonomy, and networking, with many recent developments motivated by the search of new electromagnetic counterparts to gravitational waves in the next months. This has a strong impact in many other astrophysical fields, like fireballs detection, minor planet studies, the search for extra-solar planets, the monitoring of variable stars in our Galaxy, the study of active galactic nuclei, the detection and monitoring of supernovae, and the immediate follow-up of high-energy transients such as cosmic gamma-ray bursts, besides the search of neutrino and gravitational waves electromagnetic counterparts. Last, but not least, space debris surveillance and tracking is another field of increasing interest. Educational aspects will be also covered.

Email.: astrorob@iaa.es

existing robotic observatories worldwide, new hardware and software developments, real-time analysis pipelines, wide-field imaging and follow-ups, archiving the data and quality control, telescope and observatory control systems, transient detection and classification, protocols for robotic telescopes networks, scientific results, public outreach, citizen science, global networks, educational applications, future strategies, space debris surveillance and tracking

Institut d'Astrophysique de Paris & Observatoire de Paris

The High Energy Phenomena in Relativistic Outflows (HEPRO) conferences are a cycle of biennial events devoted to the discussion of the most recent developments, either theoretical, phenomenological, or observational, on the major themes of high-energy and multi-messenger astrophysics associated with relativistic winds and jets, on all scales. Some specific themes that will be addressed at HEPRO VIII include gamma-ray and neutrino production in relativistic outflows, the environments of compact objects, the physics of relativistic sources, multi-messenger connections, and particle acceleration.

Event secretariat;     Email.: hepro8@iap.fr

high-energy astrophysics, multi-messenger astrophysics, relativistic astrophysics

The goal of this meeting is to discuss and consolidate recent advances in the vibrant research fields of string theory, holography, black hole physics, and cosmology. We will address important open problems through an active program of talks by well recognized scientific leaders in the field. In addition, we will organize an open discussion forum for researchers with close ties to the countries from the Balkan region and other parts of Eastern Europe in which we plan to brainstorm about future activities of the existing SEENET-MTP network, and other networking collaborations that will enhance the development of fundamental theoretical physics in these countries.

Qilu Normal University & Department of Education of Shandong Province &Purple Mountain Observatory, Chinese Academy of Sciences &National Supercomputing Jinan Center

Astronomy is facing the challenges and opportunities of big data. China played an important role in the development of basic disciplines of astronomy in the past two decades. Some large-scale ground-based and space-based astronomical equipments have been put into use, such as the ground-based 500-meter aperture spherical radio telescope FAST, the large-scale area multi-target optical fiber spectroscopic telescope LAMOST, the high-altitude cosmic ray observatory LHAASO, the space-based high-energy satellites DAMPE Wukong, HXMT Huiyan, GeCam Huairou-1, solar satellites Xihe and ASOS. And the chinese space station telescope CSST, Einstein EP and Sino-French cooperation satellite SVOM are preparing for launch. These large scientific equipments provide astronomical researchers with massive amounts of high-quality data, pushing astronomy research to the era of big data.

Local Organizing Committee;     Tél.: [+8613518615092];     Email.: menquan@qlnu.edu.cn

Astronomical big data analysis processing and mining, construction of China's astronomical big data processing and sharing platform, astronomical big data algorithm, radio astronomy and compact star physics

Physique numérique,    Gestion des connaissances, Big Data Computing

Banff International Research Station (BIRS) for Mathematical Innovation and Discovery

What could be a bigger source of "big data" than the entire Universe? Researchers in statistics and computer science are developing new methods to analyse the "big data" that companies and governments want to understand. To test out these methods they need big datasets that everyone can share --- and new astronomical telescopes just happen to be gearing up to generate observations of billions of stars and galaxies that fit the bill. Insights from statistics will help astrophysicists to get the most out of these observations. The Astrostatistics 2023 workshop will bring together statisticians and astrophysicists to learn the technical languages of the two fields and identify how to work together to combine the excitement of space with big data.

Statistique, Théorie des jeux,    Calcul scientifique et science des données

Frontiers in Machine Learning in Cosmology and Particle Physics 2023 is a workshop on the latest machine learning developments in the domains of cosmology and particle physics. It takes inspiration from the influential workshop series "Hammers & Nails", organised every other year by the Weizmann Institute of Science, Israel.

Réseaux de neurones et intelligence artificielle, apprentissage automatique,    Physique des hautes énergies, des particules et des champs

American Association of Variable Star Observers

The Annual Meeting of the AAVSO comprises a reception with guest speaker, Landolt Lecture, keynote speakers, research presentations, and the Membership Meeting. The conference closes with a banquet on Sunday evening. Keynotes include "40 years of Research on Cataclysmic Variables with AAVSO," presented by Dr. Paula Szkody from the University of Washington; "Looking for the Footprints of Protoplanets," presented by Dr. Katherine Espaillat from Boston University; and "Imaging Stars with the CHARA Array," presented by Dr. Gail Schaefer from Georgia State University. Presentations and the Membership Meeting will be simulcast live on Zoom. On Friday, there will be a pre-conference Python Workshop, led by Dr. Matthew Craig, requiring separate registration.

Tél.: [+1 (617) 354-0484];     Email.: aavso@aavso.org

variable stars, stellar astronomy, observing, astrophysics, protoplanets, imaging, citizen science, membership meeting

Isaac Newton Institute for Mathematical Sciences (INI)

This workshop aims to bring together researchers in solution-generating techniques and integrability, as well as Riemann-Hilbert factorization problems in gravity. It will also bring in expertise in AI and machine learning as a tool, especially in solving factorization problems, and in developing new matrix factorization methods that will be of service to solving gravitational PDEs. This event is the second workshop in a 4-month long BLH programme at the INI centred around the same topics.

Société astronomique de France, Paris Observatory, and BSN project

The International Meeting on Eclipsing Binary Star Systems (EBS) will take place in Paris, France, on November 11 and 12, 2023. The main goal of the 2023 meeting is to review eclipsing binary systems from a theoretical and observational point of view. Therefore, this meeting is planned for both professionals and amateurs. However, most of the focus of the meeting will be on the W UMa-type binary systems, which are one of the most interesting types of binary systems and are important astrophysical tools for understanding star formation, structure, and evolution. A large number of these binary systems have not been observed and analysed yet. In order to analyse these binaries, it is usually necessary to have appropriate ground-based observations at the large and small observatories. We welcome all branches regarding eclipsing binary systems. Another goal of this meeting is to establish proper communication between professionals and amateur observers in this field.

This meeting was organized by the Société astronomique de France, Paris Observatory and the BSN project. ‘English’ is the meeting language, and the number of places for face-to-face participation is limited.

Tél.: [00 (33) 1 42 24 13 74];     Email.: patrick.wullaert@saf-astronomie.fr

Binary star systems

Isaac Newton Institute for Mathematical Sciences (INI)

This workshop aims to bring together researchers in quantum gravity and in holographic quantum information to take advantage of the rapid recent progress in these streams of research with a view to tackling outstanding questions related to black hole entropy and, more generally, the structure of information in quantum gravity. This is the last of the 3 workshops of a 4-month long BLH programme at the INI centred around the same topics.

Email.: https://www.almaobservatory.org/en/alma-at-10-years-past-present-and-future/

Indian Institute of Technology Guwahati, Assam, India

The tenth edition of International Conference on Gravitation and Cosmology (ICGC) conference at IIT Guwahati aims to bring together experts working in the area of Gravitation and Cosmology to discuss the recent developments, present status and exchange ideas while providing young researchers from India an opportunity for interaction with experts. The programme will have a series of plenary lectures, with parallel and poster sessions.

Email.: icgc2023@iitg.ac.in

Classical & Quantum Gravity, Gravitational Waves, Astrophysical Relativity, Cosmology

American Astronomical Society (AAS)

One of the central features of the AAS Summer and Winter Meetings is their plenary talks spanning the full breadth of astrophysics. Some plenaries are given by prize winners from the AAS and other organizations, while other speakers are selected by the AAS Vice Presidents. Most plenary talks present science content, but talks on the state of the profession, demographics, and societal issues of relevance to the astronomical community are also regularly scheduled.

ETH Zurich

The planets that are best understood are the four terrestrial planets of our own solar system. Applying the detailed understanding gleaned from these bodies is crucial in our interpretation of exoplanetary systems. With the ongoing programs to search for planets around nearby stars, as well as upcoming ground- and space-based surveys, we can anticipate huge growth in the number and information on detected rocky exoplanets in the coming decades. As the characterisation of these new planetary systems proceeds it will in turn improve understanding of our own solar system, and in particular of how potentially habitable Earth-like planets may form, evolve, and are distributed throughout the galaxy.

The Rocky Worlds conference series aims to bring together planetary scientists, astronomers, and earth scientists to foster discussion and build the collaborations that will pave the way for the next decade of rocky exoplanet discovery and characterisation.

astronomy, exoplanets, planetary science, geophysics, geochemistry, climate science, astrobiology, origins of life

Kavli Institute for Theoretical Physics (KITP)

While it is widely acknowledged that string theory provides a framework for addressing quantum gravitational (and even quantum field theoretic) questions, the precise nature of its organizational principle remains obscure. Nearly three decades ago, when the question “What is string theory?” was asked, the perturbative string worldsheet viewpoint played the starring role. Since then, the discovery of D-branes, string dualities, and the holographic AdS/CFT correspondence has had spacetime dynamics taking center-stage. Much insight has been gleaned from these developments. We now have, for example, a much broader class of string backgrounds with better control over compactifications; strong constraints on the low energy effective field theories; a plethora of gauge-string dualities as well as applications of holographic techniques to a wide class of physical problems; and new angles on semiclassical gravitational physics from a fruitful interplay with quantum information in holography. Together with an influx of new tools and techniques, we have a very rich set of perspectives that illuminate the subject we continue to call string theory. While all these developments are interesting in and of themselves, it is an opportune moment to attempt to synthesize these, often disparate, strands and arrive at a deeper answer to the question in the title.

Physique des hautes énergies, des particules et des champs,    Physique mathématique

The goal of the seminar is to bring together global experts from experiment and theory in the field working on various storage ring projects for a constructive discussion of the most promising paths to maximize the impact of the available facilities and exploit synergies among the groups.

Physique des hautes énergies, des particules et des champs,    Accélérateurs de particules

Stars are the building blocks of our Universe. Not only do they synthetise all heavy elements such as carbon and oxygen, but they heat and energize their surrounding medium and host planets, the cradle of life. Understanding star formation is therefore of broad and fundamental interest in astrophysics and beyond. Yet it is an extremely rich multi-scale and multi-physics process which entails several fields of knowledge in interaction. The purpose of the school is to provide the newer generation of scientists working in this field with the basic knowledge necessary to carry out research in this field. Students and early postdocs are particularly welcome to register.

star formation, physical processes, gravity, turbulence, magnetic field, cooling, heating, radiative transfer, dust grains, cosmic rays, molecular clouds, interstellar medium, protoplanetary disk, galaxy, stars

UC Santa Barbara, Kavli Institute for Theoretical Physics (KITP)

Turbulence is an important process in various astrophysical environments and over vast scales. These environments range from the interior of stars, the solar wind, accretion flows, disks, jets, the interstellar medium and the circumgalactic medium, to the intra-cluster medium. The past few decades have seen great advances in both observational and theoretical studies of astrophysical turbulence. The advances in understanding and measuring turbulence have also brought significant changes to many branches of astronomy.

This conference will bring together turbulence experts from a wide range of subfields in astrophysics and physics. The goal is to encourage and enhance interdisciplinary discussions and collaborations. The conference will cover many topics, including: turbulent dynamo, magnetic reconnection, plasma physics, space physics, unresolved physics and sub-grid models in numerical simulations, turbulence in the laboratory, new observational techniques for diagnosing turbulence, connecting observations and models, and astrophysical applications of magnetized turbulence (e.g. star formation, cosmic rays, accretion, galaxy formation and evolution).

MIAPbP - Munich Institute for Astro-, Particle and BioPhysics an institute of the Excellence Cluster ORIGINS

ADONIS is aimed at investigating the chemical enrichment of nearby galaxies by using theory and observations. We plan to join efforts from world-leading experts working on resolved and unresolved stellar populations, and on state-of-the-art theoretical modelling.In case you would like either to become more familiar with these issues or to discuss recent findings on metallicity distribution and gradients youare really welcome to join us!

TESS welcomes participation by the entire Heliophysics community, including all four traditional sub-disciplines devoted to studies of the Sun, Heliosphere, Magnetosphere, and Ionosphere-Thermosphere-Mesosphere.

The Triennial Earth-Sun Summit is a joint meeting of the AAS Solar Physics Division and the Space Physics and Aeronomy Section of the American Geophysical Union.

UC Santa Barbara, Kavli Institute for Theoretical Physics (KITP)

Tidal disruption events (TDEs), which occur when a star is destroyed by the immense tidal field of a supermassive black hole, fuel luminous accretion flares that provide unique insight into the properties of galactic nuclei and their central black holes. The detection rate of these events has accelerated in recent years thanks to advances in wide-field survey capabilities across the electromagnetic spectrum. Nonetheless, there remain theoretical uncertainties in the modeling of TDEs that obfuscate understanding in the face of observations, and our ability to use TDEs as a collective Rosetta Stone for deciphering black hole demographics across cosmic time remains elusive. To bridge theory and observation and to start to tap the wealth of understanding contained within TDE observations, this conference aims to unite the diverse field of astronomers working on TDEs and the related fields of variable Active Galactic Nuclei (AGN) and X-ray binaries. This conference will highlight the recent advances that have been made in understanding TDEs, make connections to related astrophysical phenomena, and elucidate the most outstanding questions in TDE theory and observation.

MIAPbP - Munich Institute for Astro-, Particle and BioPhysics an institute of the Excellence Cluster ORIGINS

The exchange of mass, energy, and metals between galaxies, their surrounding circum-galactic medium (CGM), and the gas permeating halos at larger scale represents a fundamental part of the modern astrophysics. Both components still elude our knowledge. Indeed, we are very far from having a census of the CGM properties in the bulk of the galaxy population. Furthermore, the halo gas is well known at large scale only in the most massive halos of our Universe, the galaxy clusters (intra-cluster medium, ICM), but it is still very elusive in the bulk of the virtualized halo population at the group mass scale (Intra-group medium IGrM).

With the advent of instrument such as eROSITA, XRISM and JWST, and the enormous variety of results collected by Alma, MUSE, KCWI and LOFAR, it is time to review the state of the art of this research field. The final goal of this workshop is to fill the knowledge gap and review in an unbiased way all the key aspects of the baryon cycle: from the hot IGrM enclosed in the bulk of the virtualized halo population, to the CGM at hundreds of kpc from the central galaxy, and down to the main mechanisms in act at the galaxy center able to trigger the baryonic exchange.

American Geophysical Union (AGU)

AbSciCon brings the astrobiology community together every two years to share research, collaborate, and plan for the future. Diversity, interdisciplinary research and engaging topics make AbSciCon the premier conference for astrobiology.

Biologie,    Biochimie et chimie médicale, toxicologie

The international conference Loops ‘24 is the most recent in a long tradition of biennial meetings focused on loop quantum gravity and background independent approaches to quantum gravity. The conference will be held from Monday, May 6 through Friday, May 10, 2024, at the campus of Florida Atlantic University in Fort Lauderdale, Florida (USA). The program will feature morning plenary talks complemented by contributed talks. Plenary sessions will be held in the auditorium of the Broward County Main Library one block away from the campus. The conference will highlight recent developments in canonical loop quantum gravity, covariant loop quantum gravity (spin foams), and other approaches to quantum gravity, as well as applications to symmetry-reduced models, quantum cosmology, black holes in quantum gravity, and other topics. Foundational, mathematical, numerical and phenomenological aspects will be covered.

Gravitation and Cosmology

Physique des hautes énergies, des particules et des champs,    Physique mathématique

The IWM-EC 2024 is organized by INFN-Sezione di Catania, INFN-LNS and Dipartimento di Fisica e Astronomia "Ettore Majorana" of University of Catania. The workshop is supported by the CHIMERA and INDRA-FAZIA Collaborations.

MIAPbP - Munich Institute for Astro-, Particle and BioPhysics an institute of the Excellence Cluster ORIGINS

It is widely accepted that habitability and the capability of a planet to maintain its habitable conditions are deeply interwoven with its chemical composition and physical properties such as its atmospheric and geological/geophysical characteristics, orbital motion, dynamics, and its interactions with its host star. How these interactions originate and how they enable the planet to maintain its habitability are complex questions that can only be answered through collaborations between scientists of their respective fields. This workshop aims to bring together scientists from the fields of stellar astrophysics, planetary science, planetary dynamics, geology, and geophysics to discuss fundamental questions regarding the formation, characterization, and detection of habitable planets. Our plan is to facilitate interactions among participants through lectures, presentations and discussion sessions as well as to provide them with ample time to initiate collaborations and carry out their independent research. Our workshop is open to scientists of all levels, in particular junior and early-career researchers.

Cours et événements pour étudiants en physique,    Géophysique et géologie

UC Santa Barbara, Kavli Institute for Theoretical Physics (KITP)

Observables spanning a wide range of cosmic epochs and length-scales independently testify to the existence of dark matter. Although little is known about the microphysical nature of dark matter, its mere existence points to physics beyond the Standard Model. New developments in theory, cosmological simulations, and observational capabilities in the era of large surveys have opened up a vast landscape for dark matter discovery, which includes models that can only be tested by astrophysical and cosmological probes.

American Astronomical Society (AAS)

One of the central features of the AAS Summer and Winter Meetings is their plenary talks spanning the full breadth of astrophysics. Some plenaries are given by prize winners from the AAS and other organizations, while other speakers are selected by the AAS Vice Presidents. Most plenary talks present science content, but talks on the state of the profession, demographics, and societal issues of relevance to the astronomical community are also regularly scheduled.

The conference, along the tradition of the previous editions of the Torino workshop, will be focused on the physics and nucleosynthesis of asymptotic giant branch (AGB) stars and on several related topics. Among others, the meeting will offer a valuable opportunity to discuss the status of the art of AGB, post-AGB, super AGB modelling, the role of these stars in the chemical evolution of the Milky Way and other galaxies, the possibilities offered by present and future observational facilities (such as JWST, VLT, LAMOST, ELT ecc.), the study of dust formation in the wind of evolved stars and the meteoritic stardust measurements, hot topics in the field of theoretical and nuclear astrophysics.

The scope of the workshop is to bring together researchers from a variety of research fields, to address the current issues, and to discuss the future directions by interdisciplinary approaches. The conference program will include a series of oral presentations and poster sessions.

SPIE – The International Society for Optics and Photonics

SPIE Astronomical Telescopes + Instrumentation is the most prestigious event for developers of ground-based, airborne, and space-based telescopes, the supporting technologies, and the latest instrumentation. Taking place every two years, the 2024 conference will be held in Yokohama, Japan. No other draws the number of elite researchers, innovators, and companies, whose collective efforts push the frontiers of space and enable the building and maintaining of the important telescopes of the world.

Customer Service;     Tél.: [360-676-3290];     Email.: customerservice@spie.org

Adaptive optics, exoplanets, Interferometry, infrared, Instrumentation, spectrograph, spectroscopy, telescope, calibration, polarimetry, ELT, interferometry, wavefront sensing and distortion, diffractive optics

Optique et lasers,    Métrologie et instrumentation

MIAPbP - Munich Institute for Astro-, Particle and BioPhysics an institute of the Excellence Cluster ORIGINS

How did quantum fluctuations of the inflaton field provide the seeds for structure on cosmological scales? Did other fields play a role during inflation? How did their quantum fluctuations imprint on cosmological observables (e.g., non-Gaussianity) or survive as cosmological relics today (e.g., dark matter, matter/antimatter asymmetry)? How can these degrees of freedom be embedded into a compelling UV theory? By bringing together experts on particle physics and cosmology, we hope to develop a deeper understanding of these tough questions over the course of this 4-week MIAPbP meeting.

Cours et événements pour étudiants en physique,    Physique des hautes énergies, des particules et des champs

Galileo Galilei Institute

The neutrino oscillation discovery was a breakthrough with an impact in particle physics, astrophysics and cosmology. While most of the mixing parameters are precisely measured, key open questions remain including the neutrino absolute mass and mass ordering, the neutrino nature, the existence of CP violation in the lepton sector, of non-standard interactions and of sterile neutrinos. While the majority of the available oscillation results are understandable by considering three active neutrinos only, some anomalies are actively debated. In parallel with the progress in our knowledge of neutrino properties important advances were made in cosmology and astrophysics. Among the open problems is neutrino flavor evolution in dense astrophysical media. In particular, recent theoretical studies of dense weakly interacting many-body neutrino systems in astrophysical environments uncovered novel connections to other domains including quantum computing. Moreover, the observation of ultra-high energy neutrinos opened a new window in neutrino astronomy; while the discovery of the diffuse supernova neutrino background is expected in the foreseeable future. The goal of the workshop is to create a collaborative and brainstorming atmosphere around key open issues at the neutrino frontiers. Neutrino 2024 will take place just before the GGI program that will happen at a very timely period when running experiments might deliver first results. Crossing results from Earth experiments, astrophysics and cosmology will be a major tool to push forward progress on crucial open issues at the frontiers.

Galileo Galilei Institute

The neutrino oscillation discovery was a breakthrough with an impact in particle physics, astrophysics and cosmology. While most of the mixing parameters are precisely measured, key open questions remain including the neutrino absolute mass and mass ordering, the neutrino nature, the existence of CP violation in the lepton sector, of non-standard interactions and of sterile neutrinos. While the majority of the available oscillation results are understandable by considering three active neutrinos only, some anomalies are actively debated. In parallel with the progress in our knowledge of neutrino properties important advances were made in cosmology and astrophysics. Among the open problems is neutrino flavor evolution in dense astrophysical media. In particular, recent theoretical studies of dense weakly interacting many-body neutrino systems in astrophysical environments uncovered novel connections to other domains including quantum computing. Moreover, the observation of ultra-high energy neutrinos opened a new window in neutrino astronomy; while the discovery of the diffuse supernova neutrino background is expected in the foreseeable future. The goal of the workshop is to create a collaborative and brainstorming atmosphere around key open issues at the neutrino frontiers. Neutrino 2024 will take place just before the GGI program that will happen at a very timely period when running experiments might deliver first results. Crossing results from Earth experiments, astrophysics and cosmology will be a major tool to push forward progress on crucial open issues at the frontiers.

The International Union of Pure and Applied Physics in collaboration with Universidad de Guadalajara (Chair)

The International Symposium on Very High Energy Cosmic Ray Interactions (ISVHECRI) is a biennial conference series supported by the International Union of Pure and Applied Physics (IUPAP). Its primary objective is to provide a forum for the discussion of very high energy interactions for the interpretation of cosmic ray data based on the information available from both accelerator and cosmic ray experiments. This unique series brings together cosmic ray physicists and scientists involved with high energy accelerators and colliding beam facilities. This is the first time ISVHECRI is held in Mexico looking to benefit Latin-America and Caribbean countries.

Chair of the Local Organizing Committee;     Email.: edfuente@gmail.com

High energy astroparticle physics results relevant to particle physics, Accelerator experiments relevant to cosmic ray physics, Space experiment results relevant to high energy interactions, Exotic phenomena & searches for new physics beyond SM, LHC pp & heavy ion physics, Cross-sections and interaction models, High energy neutrinos and muons, including muon puzzle, Simulation tools for cosmic ray & neutrino physics, Multi-messenger cosmic ray observations & interpretations, Future accelerators & cosmic ray experiments

COMMITTEE ON SPACE RESEARCH (COSPAR)

Mathematisches Forschungsinstitut Oberwolfach (MFO, Oberwolfach Research Institute for Mathematics)

Casa Matemática Oaxaca (CMO)

This workshop will gather experts from around the world to discuss and unearth connections between numerical methods designed for the optimal allocation of resources, the study of fluid flow, and the nascent field of modeling the evolution of the early universe.

Mathématiques appliquées (en général),    Mathématiques numériques

UC Santa Barbara, Kavli Institute for Theoretical Physics (KITP)

The exploration of cosmic dawn is currently in an exceptionally exciting phase, and we expect the immediate future to be even more exciting with a new set of discoveries delivered by JWST. The observations of first stars, galaxies, and black holes with JWST and other facilities provide a unique “stress test” for a new generation of theoretical models of galaxy formation. The aim of the conference is to bring together theorists and observers to discuss the following key questions: What can we learn from JWST data on the nature of the first stars and black hole seeds? What is the nature of the stellar populations inhabiting the first galaxies? What are the star formation and chemical enrichment histories of early galaxies? Do we understand the key physical processes that shape the evolution of these early galaxies and their black holes? How can we connect the pictures derived from near-field and deep field observations?

UC Santa Barbara, Kavli Institute for Theoretical Physics (KITP)

The exploration of cosmic dawn is currently in an exceptionally exciting phase, and we expect the immediate future to be even more exciting with a new set of discoveries delivered by JWST. The observations of first stars, galaxies, and black holes with JWST and other facilities provide a unique “stress test” for a new generation of theoretical models of galaxy formation. The aim of the conference is to bring together theorists and observers to discuss the following key questions: What can we learn from JWST data on the nature of the first stars and black hole seeds? What is the nature of the stellar populations inhabiting the first galaxies? What are the star formation and chemical enrichment histories of early galaxies? Do we understand the key physical processes that shape the evolution of these early galaxies and their black holes? How can we connect the pictures derived from near-field and deep field observations?

MIAPbP - Munich Institute for Astro-, Particle and BioPhysics an institute of the Excellence Cluster ORIGINS

In recent years, spurred in large part by the development of first-principles numerical simulations, the plasma astrophysics community has made important strides in understanding the plasma processes relevant for astrophysical systems. The next step, which will be a key topic of the MIAPbP program, is to connect the rich plasma behavior to observed radiative phenomena. These phenomena include old puzzles, e.g. hard X-ray emission from accreting black holes, gamma-ray flares from blazars, cosmic ray acceleration, giant magnetar flares and GRBs. Plasma physics is also key to solving new puzzles such as the cosmological FRBs and gamma-rays from neutron star mergers. The role of plasma instabilities is especially prominent in transient phenomena and strong connections are emerging between plasma physics and time-domain astronomy, a quickly developing observational field. Plasma physics also plays an increasing role in multi-messenger astronomy where main targets are energetic compact objects capable of producing neutrinos, gravitational waves, and nonthermal radiation. The current efforts to understand plasma behavior lay the foundations for the future of high-energy astrophysics. Within a two-week MIAPbP program, we want to facilitate progress in this direction by bringing together both senior researchers as well as early-career scientists.

Cours et événements pour étudiants en physique,    Physique des plasmas, fusion nucléaire

Physique nucléaire,    Physique des hautes énergies, des particules et des champs

COSMO'24 will take place for October 21-25, 2024 in Kyoto, Japan. It will bring together a wide range of cosmologists and particle physicists to discuss current ideas on particle physics and cosmology.

Banff International Research Station (BIRS) for Mathematical Innovation and Discovery

Cours et évènements pour étudiants en mathématiques,    Réseaux de neurones et intelligence artificielle, apprentissage automatique

American Astronomical Society (AAS)

One of the central features of the AAS Summer and Winter Meetings is their plenary talks spanning the full breadth of astrophysics. Some plenaries are given by prize winners from the AAS and other organizations, while other speakers are selected by the AAS Vice Presidents. Most plenary talks present science content, but talks on the state of the profession, demographics, and societal issues of relevance to the astronomical community are also regularly scheduled.

One of the central features of the AAS Summer and Winter Meetings is their plenary talks spanning the full breadth of astrophysics. Some plenaries are given by prize winners from the AAS and other organizations, while other speakers are selected by the AAS Vice Presidents. Most plenary talks present science content, but talks on the state of the profession, demographics, and societal issues of relevance to the astronomical community are also regularly scheduled.

American Astronomical Society (AAS)

One of the central features of the AAS Summer and Winter Meetings is their plenary talks spanning the full breadth of astrophysics. Some plenaries are given by prize winners from the AAS and other organizations, while other speakers are selected by the AAS Vice Presidents. Most plenary talks present science content, but talks on the state of the profession, demographics, and societal issues of relevance to the astronomical community are also regularly scheduled.

American Astronomical Society (AAS)

One of the central features of the AAS Summer and Winter Meetings is their plenary talks spanning the full breadth of astrophysics. Some plenaries are given by prize winners from the AAS and other organizations, while other speakers are selected by the AAS Vice Presidents. Most plenary talks present science content, but talks on the state of the profession, demographics, and societal issues of relevance to the astronomical community are also regularly scheduled.