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Fundamental physics today

15 May 2025

Between Theory and Experiment, in search of new physics

Fundamental physics research is currently at a time of great uncertainty, but also of extraordinary fascination. For over half a century, a solid theory recognized by the scientific community has guided the design of experiments, which have consistently confirmed its predictions with great precision. The discovery of the Higgs boson in 2012 marked the completion of a long period of experimental search for new particles predicted by a theoretical model that, success after success, has become the Standard Model of elementary particles. A true journey of discoveries spanning forty years that has led to Nobel Prizes and an ever-deeper understanding of fundamental physics. From neutral currents to the Higgs boson, through the W and Z vector bosons, this has consolidated the guiding role of theory in the search for new processes and new elementary particles. Today, however, we know that the Standard Model, while it describes well the physics of particles we observe, is not considered the final framework. It is necessary to go beyond it, both through theoretical research and experimental efforts, in the quest for new physics.

Event recorded with the CMS detector in 2012 at a proton-proton centre of mass energy of 8 TeV. (© CERN)

In the brief article introducing the Standard Model, dated 1967, Steven Weinberg wrote: “Certainly, our model has too many arbitrary features for these predictions to be taken seriously.” In fact, many theoretical ideas developed during those years were incorporated into a realistic model: from the extended gauge theory of weak interactions (and later strong interactions), to spontaneous symmetry breaking and the Higgs mechanism, resulting in a number of completely new predictions, all of which at the time remained to be verified. Over time, each of these predictions has been experimentally confirmed. Today, thanks to the energy and precision of current experiments, such as those conducted at the LHC at CERN, no significant deviations from the Standard Model’s predictions are observed. Have we thus understood everything about fundamental physics? Or are we rather in a situation similar to that at the end of the 19th century, when all physics seemed to be understood before revolutions like relativity and quantum mechanics  radically changed our way of interpreting reality?

It is very difficult to draw historical parallels or predict future developments, but what is certain is that many open questions remain—questions whose answers are not found within the Standard Model. For example: are neutrinos Dirac or Majorana fermions? Why do strong interactions seem not to distinguish between matter and antimatter? How can gravity, which is very weak at the energies we can reach, be integrated with the other fundamental forces? How can we explain the instability of the mass of the Higgs boson? Why do three families of particles exist that are similar but have different masses? How is the mass spectrum of fermions in the Standard Model generated—the elementary particles that make up matter? These are just some of the questions driving scientists around the world to search for new theories and new particles.

But there is also something else: over the last hundred years, starting from Einstein’s general theory of relativity and with Lemaître’s early ideas and Hubble’s data on the expansion of the universe, a cosmological model has been developed, called the Cosmological Standard Model (or ΛCDM model), capable of describing the evolution of the universe from the very first moments after the Big Bang  up to today, reproducing its main observed features such as expansion, light element abundance, and cosmic microwave background radiation. Within this universe model, nuclear and particle physics play a fundamental role in understanding those earliest moments, inflationary epochs, and electroweak phase transitions, as well as star functioning and heavy element formation. The observation of the cosmos and the successes of this cosmological model strongly suggest that the Standard Model of particles is incomplete.

Pie chart illustrating the cosmological composition of the universe. (© INFN)

The energy budget of the universe, derived from measurements of the cosmic microwave background radiation, indicates that ordinary matter makes up less than 5% of the total, while the remaining 95% is divided between dark matter (about 25%) and dark energy (about 70%). While the nature of dark energy—some form of negative pressure responsible for the accelerated expansion of the universe—is highly speculative, dark matter, which is matter that does not emit electromagnetic radiation, can be composed of both macroscopic components, such as black holes, and microscopic ones, like elementary particles that, to explain the formation of large-scale structures in the universe, must be electrically neutral, massive, and weakly interacting. There are no particles with these characteristics within the Standard Model, so it is necessary to go beyond it—just as we need to go beyond to explain the observed matter-antimatter asymmetry in the cosmos.

Today, we face a fundamental question: do we already have a new theoretical model capable of addressing and solving some of the most important open issues, offering testable predictions for future experiments? The answer is: we do not know yet. It could be that the future Standard Model is already around the corner, with many new predictions to test, or that it already exists but we have not yet given it proper credit. At this stage, experiments are guiding us toward where particle physics will develop next. To make progress, it will be necessary to raise the energy thresholds even further, increase the intensity and sensitivity of our instruments, explore a wide range of possibilities without bias, and look for potential deviations—deviations that must exist even if we do not yet know where they are.

An example of a theory that has generated great interest and hope since the 1980s is Supersymmetry. The Minimal Supersymmetric Standard Model (MSSM) predicts rich phenomenology, with many new particles—supersymmetric partners of the particles in the Standard Model—including a possible candidate for dark matter. Additionally, it could stabilize the mass of the Higgs boson if the supersymmetric particles are not too heavy, enable new sources of matter-antimatter asymmetry, and facilitate the unification of interactions at high energies. However, despite experimental efforts, so far there have been no confirmations of the predictions of this theory. On the contrary, twenty years of research at the LHC have not found any supersymmetric particles, pushing their mass values higher and higher. Although the model cannot be completely ruled out, some of the theoretical motivations supporting it have weakened as the masses of supersymmetric particles increase. Consequently, alternative ideas have emerged to address the still open questions of the Standard Model, which today has no clear successor.

But this uncertainty should not scare us. The history of physics teaches us that the most revolutionary theories often emerge when we least expect them, and that experimental observations can surprise us. Sometimes, theory anticipates experiment, as happened with Einstein’s relativity and, to some extent, with the electroweak theory in the Standard Model; other times, it is the experiment that challenges the theory, which must then evolve to interpret the data. This was the case with quantum mechanics—think of the photoelectric effect—as well as with the theory of strong interactions, quantum chromodynamics, which later became part of the Standard Model and developed under the influence of experiments starting at SLAC  in the late 1960s. However, theoretical physics develops in many directions, many of which are not immediately testable through direct experiments but remain within the realm of ideas and concepts. Among these are studies of phenomena at energies so high that they are unreachable with current tools—such as black hole physics—where it is essential to find a synthesis between gravity and quantum mechanics, through approaches like string theory or quantum gravity. Additionally, researchers explore dualities and relationships between theories applied in different regimes or study theories in extreme limits in an attempt to simplify and understand more complex problems. No matter how far creative thinking may go, the only clearly defined limit is summarized by a famous quote from Richard Feynman: “It doesn’t matter how beautiful your theory is, it doesn’t matter how smart you are. If it doesn’t agree with experiment, it’s wrong.”

 

Research in theoretical physics at the Italian National Institute for Nuclear Physics (INFN) has a significant tradition, started with world-renowned scientists such as Enrico Fermi, Ettore Majorana, and Bruno Pontecorvo. At INFN, research in this field is coordinated by the National Scientific Committee 4, which oversees theoretical physics projects. This committee includes over 1,500 members, comprising employees and associated university researchers—the highest number among all five scientific committees of the institute. The success and international recognition of this research are evidenced by over 1,200 papers published annually in peer-reviewed international journals, as well as by the significant involvement of young researchers in training—PhD students and post-docs—who produce approximately 300 master’s theses and 70 doctoral theses each year. Scientific activity is organized into projects classified within the following scientific areas: Field and string theory (1), Phenomenology of elementary particles (2), Hadronic and nuclear physics (3), Mathematical methods (4), Astroparticle physics and cosmology (5), Statistical and applied field theory (6).

Line 1 (field and string theory) encompasses the most formal activities related to quantum field theory and string theory, as well as general relativity and theoretical and numerical approaches to strongly interacting field theories. Lines 2 (phenomenology of elementary particles), 3 (hadronic and nuclear physics), and 5 (astroparticle physics and cosmology) include, respectively, phenomenological activities related to accelerator physics within the Standard Model and beyond, nuclear physics, and astroparticle physics—covering neutrinos, dark matter and energy, and gravitational waves—in close synergy with the various experimental activities of the Institute coordinated by their respective scientific committees. Line 4 (mathematical methods), in addition to traditional mathematical physics activities, includes the foundations of quantum mechanics and the theoretical aspects of new quantum technologies applied to computers and cryptography. Finally, line 6 (statistical and applied field theory) gathers all those sectors of theoretical research—such as turbulence, complex systems, and computational biology—that, although not directly related to INFN’s core research, share techniques based on field theory with other scientific lines.

The Institute has also established for several years a National Center for Advanced Studies in Theoretical Physics, the Galileo Galilei Institute in Florence, equipped with an international scientific committee that annually selects a program of 3-4 week-long theoretical workshops on the Institute’s research topics, making it one of the first centers of its kind in Europe. In addition to workshops, the Center also offers a program of schools for doctoral students and PhD candidates.

The INFN has dedicated an important recognition to theoretical physics: in 2018, the Galileo Galilei Medal Award was established, in honor of Galileo Galilei (1564–1642), the father of the scientific method and modern physics. The Galileo Galilei Medal is awarded every two years, starting from 2019, by a special international selection committee appointed by INFN. The prize is awarded to a maximum of three scientists who, in the 25 years prior to the award date, have achieved significant results in the field of theoretical physics of fundamental interactions between elementary particles, including gravity and nuclear phenomena.

Last but not least,  we note the latest issue of INFN’s official magazine, Asimmetrie (Italian only), recently published and dedicated to the theme of physical constants, quantities that are generally not predicted but measured, serving as the point of contact between theory and the actual physical reality determined by experiments.

la medaglia Galileo Galilei dell?INFN
Galileo Galilei Medal ©INFN

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