Author Archive

Coulomb confinement in the Hamiltonian limit

Coulomb confinement in the Hamiltonian limit

Dawid S.M.; Smith W.A.; Rodas A.; Perry R.J.; Fernández-Ramírez C.; Swanson E.S.; Szczepaniak A.P.
Physical Review D, Vol. 110, Num. 094509 (2024)
Article

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Role of coherence in many-body Quantum Reservoir Computing

Role of coherence in many-body Quantum Reservoir Computing

Palacios A.; Martínez-Peña R.; Soriano M.C.; Giorgi G.L.; Zambrini R.
Communications Physics, Vol. 7, Num. 369 (2024)
Article

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Constraints on VHE gamma-ray emission of flat spectrum radio quasars with the MAGIC telescopes

Constraints on VHE gamma-ray emission of flat spectrum radio quasars with the MAGIC telescopes

Abe S.; Abhir J.; Abhishek A.; Acciari V.A.; Aguasca-Cabot A.; Agudo I.; Aniello T.; Ansoldi S.; Antonelli L.A.; Engels A.A.; Arcaro C.; Artero M.; Asano K.; Babić A.; Baquero A.; Barres de Almeida U.; Barrio J.A.; Batković I.; Bautista A.; Baxter J.; González J.B.; Bednarek W.; Bernardini E.; Bernete J.; Berti A.; Besenrieder J.; Bigongiari C.; Biland A.; Blanch O.; Bonnoli G.; Bošnjak Ž.; Bronzini E.; Burelli I.; Busetto G.; Campoy-Ordaz A.; Carosi A.; Carosi R.; Carretero-Castrillo M.; Castro
Monthly Notices of the Royal Astronomical Society, Vol. 535, (2024)
Article

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Probing Populations of Dark Stellar Remnants in the Globular Clusters 47 Tuc and Terzan 5 Using Pulsar Timing

Probing Populations of Dark Stellar Remnants in the Globular Clusters 47 Tuc and Terzan 5 Using Pulsar Timing

Smith P.J.; Hénault-Brunet V.; Dickson N.; Gieles M.; Baumgardt H.
Astrophysical Journal, Vol. 975, Num. 268 (2024)
Article

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The Institute for Neurosciences CSIC-UMH hosts the second edition of the Drosophila Spanish Meeting

The Institute for Neurosciences (IN), a joint research centre of the Spanish National Research Council (CSIC) and the Miguel Hernández University of Elche (UMH), has organised the second Spanish Drosophila Conference, a meeting that brought together the broad national scientific community using the fruit fly (Drosophila melanogaster) as a model organism to study fundamental biological processes.

Group photo of participants at the II Spanish Drosophila Meeting. Source: IN CSIC-UMH

The conference aimed to bring together Spanish researchers working with the fruit fly across a wide range of fields, from molecular and cell biology to development, neurobiology, evolution, and systems biology. Spain has a strong tradition in this field, built on the contributions of leading scientists who have driven advances in many areas of biology. In this context, the meeting sought to showcase the breadth and diversity of current research using this model organism, foster interactions among research groups, and promote the role of the next generation of scientists.

The conference, which brought together more than 100 scientists, was structured around eight scientific sessions covering key areas of current research: cell dynamics, stem cells & regeneration, morphogenesis & patterning, evolution, disease models, neuroscience, gene regulation, and physiology & ageing.

Over the three days, plenary lectures were delivered by Pau Carazo-Salas, Professor at Universitat de València; Zita Carvalho-Santos, researcher at the João Lobo Antunes Institute of Molecular Medicine (Portugal); and Sarah Bray, Professor at the University of Cambridge, all of them internationally recognised leaders in the fields of developmental biology and genetics. The meeting also included two poster sessions, which provided participants with the opportunity to present and discuss their latest results.

As part of the programme, the conference included a tribute to Antonio García-Bellido, a key figure in the development of genetics and developmental biology in Spain and an international reference in the use of Drosophila as a model organism. The session, introduced by José Carlos Pastor Pareja (IN CSIC-UMH), Antonio Baonza, and Luis Alberto Baena (both from the Severo Ochoa Molecular Biology Centre, CSIC-UAM), featured contributions from leading national and international figures in developmental biology and genetics. Speakers included Eloísa Herrera, President of the Spanish Society for Developmental Biology (SEBD); CBMSO CSIC-UAM researchers Ginés Morata and José Félix de Celis; Cassandra Extavour, President of the Genetics Society of America; and Marco Milán, President of the European Drosophila Society, who reflected on García-Bellido’s scientific legacy and his impact on the international research community.

At the local level, the conference was organised by IN researchers Javier Morante, who leads the Neuroendocrine Control of Organ Growth and Sexual Maturation laboratory; José Carlos Pastor Pareja, head of the Cell-to-tissue Architecture in the Nervous System laboratory; and Juan Antonio Sánchez Alcañiz, who leads the Neurogenetic Bases of Behaviour laboratory.

More information at the official website: https://drosospain.umh.es/

Source: Institute for Neurosciences CSIC-UMH (in.comunicacion@umh.es)

La entrada The Institute for Neurosciences CSIC-UMH hosts the second edition of the Drosophila Spanish Meeting se publicó primero en Instituto de Neurociencias de Alicante.

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Pathways Autumn School 2026 opens applications with ICTA-UAB participation

Applications open for Pathways Autumn School 2026, featuring ICTA-UAB researcher Victoria Reyes-García on the organising committee

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The III Libro Blanco de las Nanotecnologías, Presented in Barcelona

This document, produced by the SustainableNano network (SNSSN) with strong participation from ICN2 researchers, offers a broad perspective on the role of nanotechnology in addressing major global challenges in the coming decades.

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Tracking Jet Streams as Coherent Structures: A New Mathematical Approach

A new method redefines how scientists can track jet streams, the high-altitude currents that shape weather patterns worldwide. Called JetLag, the algorithm treats jets as coherent structures in the flow of air rather than simply fast winds, recovering 85 years of atmospheric history with no hand-tuned parameters and a sensitivity to its settings more than fifty times lower than existing approaches.

When a large wildfire sends smoke into the upper atmosphere, something odd happens. The smoke does not spread evenly. It stretches along a narrow corridor, curving and bending for thousands of kilometres, and on one side of that corridor, the air stays clean. The boundary is sharp, visible from space, and it follows the path of a jet stream.

Jet streams sit roughly ten kilometres above the surface. They are fast, persistent currents of air that wrap around the planet in sinuous bands, shaping the weather systems that reach us on the ground, from winter storms to summer heatwaves. Jets play a central role in weather and climate.

How to find them is another story.

A study published in Communications Earth & Environment, co-authored by Louis Rivoire (Massachusetts Institute of Technology), Jezabel Curbelo (Full Professor at Universitat Politècnica de Catalunya, CRM affiliated researcher and 2025 Premio Nacional de Investigación laureate), and Marianna Linz (Harvard University), proposes a different way to track these currents. Their method, called JetLag, deviates from the conventional approach of looking for fast winds and instead treats jet streams as coherent structures in the flow of air, capturing their behaviour as transport barriers that separate distinct air masses over time. It proposes a different way to track these currents.

“Trying to follow the same atmospheric features using these Eulerian methods was hopeless. The atmosphere is simply too noisy.”

The standard way to locate a jet is to define it as a maximum of wind speed at a given point in the atmosphere. This is the Eulerian perspective, named after the eighteenth-century mathematician Leonhard Euler: it describes the flow at fixed points in space. The problem, as the paper illustrates, is that these wind maxima can jump between locations from one time step to the next, producing a physically implausible picture of the jet. A powerful wind created by air flowing over a mountain, for instance, can register as a jet even where no coherent stream exists. Meanwhile, regions with lower wind speeds that nonetheless support long-range transport get overlooked entirely.

“Trying to follow the same atmospheric features using these Eulerian methods was hopeless,” Rivoire says. “The atmosphere is simply too noisy.”

Instead of measuring speed at fixed locations, the Lagrangian perspective (named after Joseph-Louis Lagrange) follows individual parcels of air as they move over several days. In this view, the jet stream is the corridor where air parcels travel the farthest. Wildfire smoke makes these corridors visible: the smoke is constrained by the jet, and stays on one side of it. As the paper puts it, jets act as transport barriers, material surfaces that remain coherent by resisting stretching and filamentation. A method that captures this barrier function needs to account for how air moves over time.

Comparing Eulerian and Lagrangian views of the atmosphere on the same day. Left: wind speed field with jet detections (black dots) scattered along regions of fast wind, leaving gaps where speed drops below the detection threshold. Right: the Lagrangian displacement field (the M descriptor), where brighter colours indicate greater air parcel displacement over several days. The jet axes (black lines) trace continuous ridges of maximum displacement in both hemispheres, capturing coherent structure that the wind-based approach fragments. Animation courtesy of Louis Rivoire.

Atmospheric scientists have been tracking jets for decades using dozens of different algorithms. These methods have yielded a robust understanding of many aspects of jet behaviour and have been applied across climate science, weather forecasting and atmospheric chemistry. But they also disagree with one another in ways that carry real consequences. Different studies use different wind speed thresholds to decide what counts as a jet: 25.7 metres per second in some, 30 in others, 40 in yet others. Changing a threshold by 25 per cent can shift the estimated average latitude of the subtropical jet by about two degrees (roughly 200 km), enough to affect conclusions about long-term trends.

In a field trying to determine whether jet streams are migrating poleward under climate change, that sensitivity is hard to live with.

As Rivoire explains, “jets are not simple objects with sharp boundaries, because wind varies smoothly in space and time.” You cannot draw a line around a jet the way you draw a coastline on a map. The working framing for most of the past century has been that jets are long, narrow and wavy, but those are qualitative descriptions, and the moment you try to turn them into rules a computer can follow, choices multiply. How narrow is narrow? How fast is fast enough? Different research groups have answered differently, and their results reflect it.

On top of that, different kinds of jets arise from different physical mechanisms. The subtropical jet is relatively steady, driven by planetary rotation and the temperature gradient between the equator and the poles. Mid-latitude jets are shaped by large storm systems and shift more erratically. Most identification methods are tailored to one type or the other. JetLag works for both.

 

A mathematician and a climate scientist walk into the CRM

The project started because Rivoire needed reliable jet coordinates for another study. He was a postdoctoral fellow at Harvard, and the available methods kept giving him axes that jumped between different air masses from one time step to the next. What he wanted was continuity: a line through the atmosphere that followed the same weather features over time. Then Jezabel Curbelo visited from the Universitat Politècnica de Catalunya.

Curbelo’s research sits at the intersection of dynamical systems theory and geophysical fluid dynamics: she studies transport, mixing and stirring in the ocean and atmosphere using Lagrangian methods. She brought a different vocabulary to the problem. Where Rivoire saw atmospheric circulation, Curbelo saw trajectories, phase spaces, and coherent structures. “Our expertise was complementary every step of the way,” Rivoire says.

The Lagrangian descriptor they chose is called M. It works by releasing fictitious air parcels at every point in the atmosphere, like Chinese lanterns, letting them travel forward and backwards in time along surfaces of constant entropy (isentropes, in the jargon), and measuring how far each one goes. Ridges in the resulting map of displacement, the places where parcels travel farthest, reveal the jet.

Why ℳ over other Lagrangian tools?

Alternatives like finite-time Lyapunov exponents (FTLEs) require computing a Jacobian matrix and need very fine grids. For a dataset covering over eight decades of 6-hourly atmospheric data, ℳ was the only realistic option. “Several versions of the descriptor ℳ can be calculated based on the acceleration, velocity, or kinetic energy in the flow. Because jet streams are associated with sustained high-velocity regions, we chose a descriptor based on the velocity.”

Rivoire secured a grant through the CRM’s International Programme for Research Groups and came to Barcelona. The computational groundwork was done: over eight billion fictitious trajectories, computed on high-performance systems. What remained was harder.

How do you extract a jet from that data?

The jet was visible by eye in the visualisations, a bright ridge winding around the planet. Getting a computer to see it was another matter. They worked through a catalogue of extraction techniques, from edge detection to hierarchical segmentation to shortest-path algorithms. At one point, they were feeding atmospheric data into hydrological software built to trace watersheds, which gives a sense of how far afield the search went. “I started thinking that we would have to give up on a significant part of the innovation,” Rivoire says.

The key insight came during late sessions at CRM. Every technique they had tried worked locally, picking up fragments of the ridge at individual points. But jets are not local objects. What Rivoire and Curbelo call “the backbone of the atmosphere” could only be recovered as a single coherent structure, using information from the entire flow field at once, with geophysical theory setting the bounds on how much the structure could meander. “Spending a month at CRM allowed me to focus and think deeply about a complex project on which progress had been brought to a halt by other priorities,” Rivoire says. “Zoom meetings are better than nothing… but nothing beats interacting in person, chatting over lunch, immersing yourself in the work and spending an uninterrupted chunk of time thinking about one thing, and one thing only.”

Working in Barcelona was a fantastic professional opportunity, as it allowed me to make new connections,” he adds. “Between the green and quiet UAB campus and the bustling, colourful Barcelona centre, I had a fantastic time full of interesting new experiences. I would do it again in a heartbeat!”

 

Greedy algorithms and Rossby waves

The technique they arrived at is called penalised forward-backward greedy selection. The algorithm steps through longitudes, connecting locally strong features (the “greedy” part), then removes connections that weaken overall coherence (the “backward” pass). A penalty term keeps undulations within theoretical bounds set by the physics of Rossby waves, the large-scale atmospheric waves that give jet streams their sinuous shape. Rossby waves propagate westward relative to the background flow and are responsible for the familiar looping patterns in weather maps. Their typical wavelength constrains how much the jet can meander between adjacent longitudes, and that constraint is what sets JetLag’s penalty parameter. Unlike conventional methods, both of JetLag’s parameters come from theory.

The comparison with existing methods produced the paper’s most notable number. Changing JetLag’s integration time (the period over which fictitious air parcels travel) by as much as 66 per cent shifts the estimated jet position by less than 0.1 degrees on average. A 25 per cent change in the wind speed threshold used by a standard Eulerian method shifts it by roughly two degrees. More than fifty times more sensitive. “We were still surprised that the stability was so large for a system as dynamic and complex as the atmosphere,” Rivoire says.

When you study whether jet streams are shifting over decades, you need a method whose results don’t quietly depend on parameter choices calibrated to a particular climate state. A fixed wind speed threshold that works for the 1950s atmosphere might not mean the same thing in a warmer future. JetLag’s parameters are grounded in physics, which makes them portable across climates. The algorithm also runs on a standard laptop, despite working with a dataset spanning 1941 to 2024.

 

What the jet carries

Curbelo sees the collaboration as part of something she values about working between disciplines. “The language of dynamical systems provides a natural bridge,” she says. “Many phenomena in geoscience can be understood in terms of trajectories, stability and long-term behaviour, which are all central concepts in dynamical systems. At the same time, these applications raise new questions that push the theory forward.” The feedback, she argues, runs both ways. “Interdisciplinary collaborations are also very enriching on a personal level. I learn a lot from them, and I really enjoy discovering new ideas and perspectives.”

The two researchers are now using JetLag to investigate how jet streams are evolving in a warming climate and how those changes connect to extreme weather. They are also running idealised climate simulations to deepen their understanding of the underlying dynamics. One question on Rivoire’s mind concerns the path of storms over the Atlantic and Pacific, which typically tilts from southwest to northeast. That tilt determines weather impacts across populated regions. This line of work is currently underway at the Weizmann Institute of Science, where Rivoire is studying how jet streams interact with storms.

“Are storm tracks tilted because storms themselves are carving out slanted paths, or are storms mere passengers of a jet stream that’s being reshaped by the geography of continents?”

The JetLag dataset (6-hourly jet axes for both hemispheres, 1941 to 2025) and the algorithm’s code are publicly available. For a more personal account of how the research developed, Louis Rivoire’s “Behind the Paper” blog post is recommended reading.

Reference: L. Rivoire, J. Curbelo, M. Linz. Tracking jet streams as Lagrangian objects. Communications Earth & Environment 7, 267 (2026). https://doi.org/10.1038/s43247-026-03262-z

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The post Tracking Jet Streams as Coherent Structures: A New Mathematical Approach first appeared on Centre de Recerca Matemàtica.

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Desgranando FEST brings nine days of science outreach to Granada with 139 speakers and 90 activities

It takes place from April 18 to 26, with the aim of bringing science to the entire Granada region in all possible formats: workshops, film, talks, exhibitions, routes, art or critical thinking among other activities

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A global collaboration reaches 1% precision on the local expansion rate of the Universe

Image
Conceptual overview of the Local Distance Network, a multi-route approach to deriving the Hubble constant in our universe. Included are a non-exhaustive collection of various methods for determining galactic distances and how these can connect the absolute scale established through geometric means to the Hubble constant H0. Background rectangles illustrate the positions of Rung 1, Rung 2 and Rung 3 in a traditional distance ladder from left to right.  The graphic was developed within the framework of the IS
Credits
Fabio Crameri, CC BY-SA 4.0
English

An international collaboration of astronomers has achieved the most precise direct measurement to date of the current expansion rate of the Universe. In a paper to be published in Astronomy & Astrophysics, the H0 Distance Network (H0DN) Collaboration reports a value of the Hubble constant of H₀ = 73.50 ± 0.81 km s⁻¹ Mpc⁻¹, corresponding to a precision of just over 1%.

The study, “The Local Distance Network: a community consensus report on the measurement of the Hubble constant at 1% precision, is the outcome of a broad community effort launched at the ISSI Breakthrough Workshop What’s under the H0od?, held at the International Space Science Institute (ISSI) in Bern in March 2025.

A network, not a single path

For nearly a century, astronomers have relied on the “distance ladder” to measure the Hubble constant, H0H_0H0​, by calibrating increasingly distant cosmic objects through a sequence of interlocking steps. While remarkably successful, this approach can allow uncertainties to propagate along a single dominant measurement path.

The H0DN Collaboration adopted a different strategy: a Local Distance Network that replaces a single ladder with a mathematical framework connecting many distance indicators simultaneously. The network links independent and overlapping distance probes — including Cepheid variables, the Tip of the Red Giant Branch (TRGB), Mira variables, megamasers, Type Ia and Type II supernovae, surface brightness fluctuations, the Tully–Fisher relation, and the Fundamental Plane — into one coherent analysis.

By explicitly accounting for correlations and shared uncertainties through full covariance weighting, the network allows the internal consistency of the entire system to be tested transparently for the first time.

“This approach shifts the focus from defending individual methods to understanding how the full ecosystem of distance measurements fits together,” says Licia Verde (ICREA–ICCUB), member of the H0DN Collaboration and Scientific Director of the ICCUB.

Robust, transparent, and community-driven

Nearly 40 experts in distance measurements and cosmology, representing a wide range of institutions and methodological backgrounds, participated directly in the ISSI workshop, with additional contributors joining remotely. Before any calculations were carried out, participants voted on the set of first-rank distance indicators, gold standards for defining a baseline solution, along with predefined variants to test robustness.

The network analysis shows that:

  • Independent distance indicators are mutually consistent within their stated uncertainties and with no outliers
  • No single method or indicator dominates the final result.
  • Removing or replacing key components – such as Cepheids, TRGB, or Type Ia supernovae – produces only minor changes in the inferred value of H₀.

To encourage scrutiny and reuse, the collaboration is releasing open-source software and data products, allowing anyone to reproduce the analysis, explore alternative assumptions, or incorporate future measurements as new data become available.

Putting the Hubble tension in context

The new local measurement remains in significant disagreement with values inferred from observations of the early Universe — such as the cosmic microwave background (CMB) and baryon acoustic oscillations (BAO) — when interpreted within the standard ΛCDM cosmological model. The discrepancy reaches approximately 5–7 standard deviations, reinforcing what is known as the Hubble tension.

Researchers from ICCUB (Institute of Cosmos Sciences of the University of Barcelona), including Licia Verde and Héctor GilMarín (ICCUBIEEC), brought to the collaboration extensive expertise in cosmology, galaxy surveys, BAO, and the CMB precisely the observations that underpin the other determination of the Hubble constant.

“Our contribution was not to champion one side of the tension,” explains Héctor GilMarín, but to rigorously assess systematic uncertainties, compare datasets, and examine whether the discrepancy points to new physics or to unresolved measurement issues.

Because ICCUB researchers are not directly involved in producing the distanceladder observations used in H0DN, they were able to play a distinct role within the collaboration.

“That external perspective allowed us to help uncover hidden assumptions and act, when needed, as neutral arbiters,” adds Verde. “We represented the viewpoint of the cosmology and earlyUniverse community within a collaboration focused on local measurements.

Rather than identifying a single problematic measurement, the distancenetwork result strengthens the case that the tension cannot be explained by a lone overlooked systematic in the local distance scale.

A foundation for future precision cosmology

Beyond delivering the most precise direct measurement of the Hubble constant to date, the Local Distance Network establishes a flexible and extensible framework for the future. With a flood of new observatories, improved calibrations, and additional geometric distance anchors becoming available, they can be integrated into the network to further refine our understanding of cosmic expansion and provide clues about the resolution of the Hubble tension

“This work shows that explanations invoking a single overlooked systematic in local distance measurements are increasingly difficult to sustain,” the authors conclude. “If the tension reflects real physics, it may indicate new ingredients beyond the standard cosmological model or require a reassessment of early-Universe inferences.”

The study also highlights the role of ISSI Bern in fostering open, collaborative, and methodologically rigorous science that bridges traditional disciplinary and institutional boundaries.

The full paper will appear in Astronomy & Astrophysics. Upon acceptance, the analysis code will be made publicly available via GitHub and the Astrophysics Source Code Library.

Original press release text by Fabio Crameri (ISSI) in collaboration with the authors.

 

Reference:

a { text-decoration: none; color: #464feb; } tr th, tr td { border: 1px solid #e6e6e6; } tr th { background-color: #f5f5f5; }

H0DN Collaboration, Casertano, S. et al. (2026). The Local Distance Network: A community consensus report on the measurement of the Hubble constant at ∼1% precision. Astronomy & Astrophysics (forthcoming).
https://doi.org/10.1051/0004-6361/202557993

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A global collaboration reaches 1% precision on the local expansion rate of the Universe

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Alejo Efeyan recibe un Programa CRIS de Excelencia para desentrañar los efectos de la restricción dietética en la prevención y el tratamiento del cáncer de hígado

Alejo Efeyan recibe un Programa CRIS de Excelencia para desentrañar los efectos de la restricción dietética en la prevención y el tratamiento del cáncer de hígado

Alejo Efeyan, jefe del Grupo de Metabolismo y Señalización Celular del Centro Nacional de Investigaciones Oncológicas (CNIO), ha recibido de la Fundación CRIS Contra el Cáncer un Programa CRIS de Excelencia, dirigido a «investigadores con proyectos revolucionarios, con alto potencial de impacto clínico».

El proyecto liderado por Efeyan se titula Dissection of protective molecular players in dietary restriction and their modulation against hepatocellular carcinoma, y está dotado con 1.250.000 de euros para cinco años.

El proyecto busca, en última instancia, avanzar hacia estrategias basadas en la dieta para prevenir en población de riesgo, y tratar el tipo más común de cáncer de hígado.

En concreto, el grupo de Efeyan en el CNIO investigará los factores moleculares implicados en los beneficios de las intervenciones de restricción calórica, para abrir el camino hacia una vía clínica para su uso terapéutico en pacientes con carcinoma hepatocelular y en la población de riesgo.

El investigador del CNIO Alejo Efeyan, en su laboratorio. /MadMoviex. CNIO

Este tipo de tumor está muy asociado al peso corporal, debido en parte a que la sobrecarga crónica de nutrientes provoca daño metabólico y disfunción de los hepatocitos. En este sentido, varios estudios preclínicos y epidemiológicos han demostrado que la restricción dietética puede ser eficaz para prevenir y tratar el carcinoma hepatocelular; sin embargo, aprovechar estos efectos beneficiosos en la clínica es complejo, tanto por lo difícil que resulta cumplir este tipo de dieta como por el desconocimiento sobre los factores moleculares y metabólicos implicados.

El proyecto financiado por CRIS Contra el Cáncer plantea que las vías de detección y señalización de nutrientes y hormonas en los hepatocitos median los efectos beneficiosos de la restricción dietética, y que el análisis detallado de los factores específicos en estas vías puede allanar el camino para diseñar fármacos que imitan la restricción dietética.

CRIS Contra el Cáncer explica que sus programas son evaluados por comités científicos independientes y externos, lo que «permite identificar y apoyar los proyectos con mayor potencial para transformar el abordaje del cáncer y acelerar la transferencia de los avances al paciente».

Sobre la Fundación CRIS Contra el Cáncer

La Fundación CRIS Contra el Cáncer -Cancer Research & Innovation in Science- es una organización independiente, apolítica, sin ánimo de lucro y con el objetivo de curar el cáncer a través de la investigación con el apoyo de la sociedad civil. Tiene sede en España, Reino Unido y Francia. Ha financiado proyectos en 107 centros de investigación de todo el mundo. En España cuenta con unidades propias de terapias y ensayos clínicos en los principales hospitales de la sanidad pública.

La entrada Alejo Efeyan recibe un Programa CRIS de Excelencia para desentrañar los efectos de la restricción dietética en la prevención y el tratamiento del cáncer de hígado se publicó primero en CNIO.

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Comunicado del Patronato del CNIO

Laura M. Lombardía / CNIO

Reunido en sesión extraordinaria el 10 de abril del 2026, ha decidido ratificar por mayoría absoluta la candidatura de Cristina Navarro Enterría para la dirección de gerencia de dicha fundación, convirtiéndose así en la primera mujer que se pone al frente de esta dirección del CNIO.

Cristina es Licenciada en Derecho por la Universidad de Barcelona, y posee también el título de Experto en Gestión de Servicios Sociales de la Universidad Complutense de Madrid. Es, además, Técnico Superior en Prevención de Riesgos Laborales, con las tres especialidades de Seguridad en el Trabajo, Higiene Industrial y Ergonomía y Psicosociología aplicada.

Como funcionaria de carrera, posee más de 25 años de experiencia en los tres niveles territoriales de la administración (local, autonómica y general), y ha desarrollado su actividad en todas las áreas gerenciales de las entidades del Sector Público Institucional: tramitación normativa, gestión económico-presupuestaria, recursos humanos, así como las relaciones entre departamentos y gestión de fondos europeos.

Ha ocupado cargos de la más alta responsabilidad en la Administración General del Estado, siendo Subsecretaria del Ministerio de Inclusión, Seguridad Social y Migraciones entre los años 2023 y 2026. Actualmente, es vocal asesora del Ministerio de Hacienda.

Este Patronato considera que Cristina Navarro reúne tanto la experiencia como la capacitación técnica óptimas para un puesto de la máxima exigencia personal y profesional, ya que cuenta no solo con una sólida trayectoria como gestora, sino que también posee la capacidad de liderazgo que requiere la dirección administrativa del mayor centro de investigación en oncología de nuestro país.

La entrada Comunicado del Patronato del CNIO se publicó primero en CNIO.

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