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Model Choice and Crucial Tests. On the Empirical Epistemology of the Higgs Discovery

Our paper discusses the epistemic attitudes of particle physicists on the discovery of the Higgs boson at the Large Hadron Collider (LHC). It is based on questionnaires and interviews made shortly before and shortly after the discovery in 2012. We show, to begin with, that the discovery of a Standard Model (SM) Higgs boson was less expected than is sometimes assumed. Once the new particle was shown to have properties consistent with SM expectations - albeit with significant experimental uncertainties -, there was a broad agreement that 'a' Higgs boson had been found. Physicists adopted a twopronged strategy. On the one hand, they treated the particle as a SM Higgs boson and tried to establish its properties with higher precision; on the other hand, they searched for any hints of physics beyond the SM. This motivates our first philosophical thesis: the Higgs discovery, being of fundamental importance and establishing a new kind of particle, represented a crucial experiment if one interprets this notion in an appropriate sense. By embedding the LHC into thetradition of previous precision experiments and the experimental strategies thus established, Duhemian underdetermination is kept at bay. Second, our case study suggests that criteria of theory (or model) preference should be understood as epistemic and pragmatic values that have to be weighed in factual research practice. The Higgs discovery led to a shift from pragmatic to epistemic values as regards the mechanisms of electroweak symmetry breaking. Complex criteria, such as naturalness, combine epistemic and pragmatic values, but are coherently applied by the community.

physics.hist-ph↗

Computability and Physical Theories

The familiar theories of physics have the feature that the application of the theory to make predictions in specific circumstances can be done by means of an algorithm. We propose a more precise formulation of this feature --- one based on the issue of whether or not the physically measurable numbers predicted by the theory are computable in the mathematical sense. Applying this formulation to one approach to a quantum theory of gravity, there are found indications that there may exist no such algorithms in this case. Finally, we discuss the issue of whether the existence of an algorithm to implement a theory should be adopted as a criterion for acceptable physical theories.

gr-qc↗

The Impact Of World War I On Relativity: Part III, The Aftermath

Neither the world nor science came to an end when the gunfire stopped on 11 November 1918 (close to 11 AM in some time zone), but neither would ever be the same again. Part I of this inquiry (Observatory 138, 46-58, April 2018) looked at the development of general relativity under the Rubric of Gerald Holton's "Only Einstein, only there, only then." Part II (Observatory 138, 98 116, June, 2018) addressed the activities, relativistic, classical, and otherwise of many (mostly) physicists who were interacting with Einstein, working on relativistic gravity, or, sometimes, against it, and leaving tracks that can still be followed. Part III considers some of what happened to Einstein, his theory of gravity, and related science after the war and, perhaps, because of it. A subset of the items will probably be familiar -- the 1919 eclipse expedition and the founding of the International Astronomical Union the same year, Einsteins 1921 Nobel Prize (for the discovery of the law of the photoelectric effect). Others perhaps less so, including a flood of books about GR (pro and con) with the end of paper rationing surely playing a role, AE's 1922 trip to Paris, and the gory details, swings and roundabouts of gravitational radiation/waves and the cosmological constant. It is left as an exercise for the reader to decide which items are primarily scientific and which primarily political. The long-range issues of "is general relativity the right theory of gravity?" and "do we have better wars?" come at the end. And I am going to start in a slightly improbable place.

physics.hist-ph↗

The strange case of Dr. Petit and Mr. Dulong

The Dulong-Petit limiting law for the specific heats of solids, one of the first general results in thermodynamics, has provided Mendeleev with a powerful tool for devising the periodic table and gave an important support to Boltzmann's statistical mechanics. Even its failure at low temperature, accounted for by Einstein, paved the way to the the quantum mechanical theory of solids. These impressive consequences are even more surprising if we bear in mind that, when this law was announced, thermal phenomena were still explained using Lavoisier's concept of caloric and Dalton's atomic theory was in its infancy. Recently, however, bitter criticisms charging Dulong and Petit of `data fabrication' and fraud, have been raised. This work is an attempt to restore a more balanced view of the work performed by these two great scientists and to give them back the place they deserve in the framework of the development of modern science.

physics.hist-ph↗

A Precipice Below Which Lies Absurdity? Theories without a Spacetime and Scientific Understanding

While the relation between visualization and scientific understanding has been a topic of long-standing discussion, recent developments in physics have pushed the boundaries of this debate to new and still unexplored realms. For it is claimed that, in certain theories of quantum gravity, spacetime 'disappears': and this suggests that one may have sensible physical theories in which spacetime is completely absent. This makes the philosophical question whether such theories are intelligible, even more pressing. And if such theories are intelligible, the question then is how they manage to do so. In this paper, we adapt the contextual theory of scientific understanding, developed by one of us, to fit the novel challenges posed by physical theories without spacetime. We construe understanding as a matter of skill rather than just knowledge. The appeal is thus to understanding, rather than explanation, because we will be concerned with the tools that scientists have at their disposal for understanding these theories. Our central thesis is that such physical theories can provide scientific understanding, and that such understanding does not require spacetimes of any sort. Our argument consists of four consecutive steps: (a) We argue, from the general theory of scientific understanding, that although visualization is an oft-used tool for understanding, it is not a necessary condition for it; (b) we criticise certain metaphysical preconceptions which can stand in the way of recognising how intelligibility without spacetime can be had; (c) we catalogue tools for rendering theories without a spacetime intelligible; and (d) we give examples of cases in which understanding is attained without a spacetime, and explain what kind of understanding these examples provide.

physics.hist-ph↗

Isaac Thuret: celebrated craftsman denied intellectual credit

The Scientific Revolution sweeping through seventeenth-century Europe led to unprecedented intellectual and scientific insights and high-profile technological developments. Combined with a significant worldwide increase in naval commerce, solving the intractable "longitude problem" became an ever more urgent requirement for the continent's main sea-faring nations. Christiaan Huygens, one of the brightest contemporary natural philosophers, established a fruitful professional collaboration with the Parisian master clockmaker Isaac Thuret. Their joint efforts eventually led to the construction of the first accurate, spring-driven watches. Despite clear evidence of Thuret's intellectual contributions, but in the absence of a robust intellectual property rights framework, Huygens insisted on claiming the invention's sole ownership. Thuret, the celebrated craftsman who had contributed crucial advice to realize the novel watch design, was thus forever--and wholly undeservedly--marked as the "invisible technician."

physics.hist-ph↗

Can Somebody Please Say What Gibbsian Statistical Mechanics Says?

Gibbsian statistical mechanics (GSM) is the most widely used version of statistical mechanics among working physicists. Yet a closer look at GSM reveals that it is unclear what the theory actually says and how it bears on experimental practice. The root cause of the difficulties is the status of the Averaging Principle, the proposition that what we observe in an experiment is the ensemble average of a phase function. We review different stances toward this principle, and eventually present a coherent interpretation of GSM that provides an account of the status and scope of the principle.

cond-mat.stat-mech↗

Levels of spacetime emergence in quantum gravity

We explore the issue of spacetime emergence in quantum gravity, by articulating several levels at which this can be intended. These levels correspond to the reconstruction moves that are needed to recover the classical and continuum notion of space and time, which are progressively lost in a progressively deeper sense in the more fundamental quantum gravity description. They can also be understood as successive steps in a process of widening of the perspective, revealing new details and new questions at each step. Each level carries indeed new technical issues and opportunities, and raises new conceptual issues. This deepens the scope of the debate on the nature of spacetime, both philosophically and physically.

physics.hist-ph↗

The Logos Categorical Approach to Quantum Mechanics: III. Relational Potential Coding and Quantum Entanglement Beyond Collapses, Pure States and Particle Metaphysics

In this paper we consider the notion of quantum entanglement from the perspective of the logos categorical approach [26, 27]. Firstly, we will argue that the widespread distinctions, on the one hand, between pure states and mixed states, and on the other, between separable states and entangled states, are completely superfluous when considering the orthodox mathematical formalism of QM. We will then argue that the introduction of these distinctions within the theory of quanta is due to another two completely unjustified metaphysical presuppositions, namely, the idea that there is a "collapse" of quantum states when being measured and the idea that QM talks about "elementary particles". At distance from these distinctions and taking the logos approach as a standpoint, we will propose an objective formal account of the notion of entanglement in terms of potential coding which introduces the necessary distinction between intensive relations and effective relations. We will also discuss how this new definition of entanglement provides an anschaulich content to this --supposedly "spooky"-- quantum relational feature.

quant-ph↗

Clifford's attempt to test his gravitation hypothesis

Almost half a century before Einstein expounded his general theory of relativity, the English mathematician William Kingdon Clifford argued that space might not be Euclidean and proposed that matter is nothing but a small distortion in that spatial curvature. He further proposed that matter in motion is not more than the simple variation in space of this distortion. In this work, we conjecture that Clifford went further than his aforementioned proposals, as he tried to show that matter effectively curves space. For this purpose he made an unsuccessful observation on the change of the plane of polarization of the skylight during the solar eclipse of December 22, 1870 in Sicily.

physics.hist-ph↗

The Computable Universe: From Prespace Metaphysics to Discrete Quantum Mechanics

The central idea of this work is the concept of prespace, a hypothetical structure that is postulated to underlie the fabric of space or space-time. I consider how such a structure could relate to space and space-time, and the implications of the existence of this structure for quantum theory. I compare space and space-time to other spaces used in physics, such as configuration space, phase space, and Hilbert space. I support the 'property view' of space, opposing both the traditional views of space and space-time, substantivalism and relationism. I argue that configuration space has a special status in the microscopic world similar to the status of position space in the macroscopic world. The prespace structure is compared with a computational system, in particular to a cellular automaton, in which space and all physical quantities are broken into discrete units. One way open for a prespace metaphysics can be found if physics is made fully discrete. I suggest as a heuristic principle that the physical laws of our world are such that the computational cost of implementing those laws on an arbitrary computational system is minimized. I discuss the 'measurement problem' of quantum mechanics. Considering how quantum theory could be made fully discrete leads naturally to a suggestion of how standard linear quantum mechanics could be modified to give a solution to the measurement problem, calling this model Critical Complexity Quantum Mechanics (CCQM). I compare CCQM with some other proposed solutions to the measurement problem, in particular, the spontaneous localization model of Ghirardi, Rimini, and Weber. Finally, I argue that the measure of the complexity of quantum mechanical states introduced in CCQM also provides a new definition of entropy for quantum mechanics, and suggests an objective foundation for statistical mechanics, thermodynamics, and the arrow of time.

quant-ph↗

My life with GianCarlo Ghirardi, a great friend, a great teacher and a great physicist

In these shorts notes I want to remembermy relationship with GianCarlo Ghirardi, who was my supervisor in my Master Degree in Physics at the University of Trieste and then he became a very deep and close friend. I don't want to describe in details his scientific steps in the world of modern Physics: many others will make better than me. I want only to share which was my relationship with him as a teacher, a man, and expecially as a deep friend, for more than 40 years.

physics.hist-ph↗

Yes, Aboriginal Australians Can and Did Discover the Variability of Betelgeuse

Recently, a widely publicized claim has been made that the Aboriginal Australians discovered the variability of the red star Betelgeuse in the modern Orion, plus the variability of two other prominent red stars: Aldebaran and Antares. This result has excited the usual healthy skepticism, with questions about whether any untrained peoples can discover the variability and whether such a discovery is likely to be placed into lore and transmitted for long periods of time. Here, I am offering an independent evaluation, based on broad experience with naked-eye sky viewing and astro-history. I find that it is easy for inexperienced observers to detect the variability of Betelgeuse over its range in brightness from V = 0.0 to V = 1.3, for example in noticing from season-to-season that the star varies from significantly brighter than Procyon to being greatly fainter than Procyon. Further, indigenous peoples in the Southern Hemisphere inevitably kept watch on the prominent red star, so it is inevitable that the variability of Betelgeuse was discovered many times over during the last 65 millennia. The processes of placing this discovery into a cultural context (in this case, put into morality stories) and the faithful transmission for many millennia is confidently known for the Aboriginal Australians in particular. So this shows that the whole claim for a changing Betelgeuse in the Aboriginal Australian lore is both plausible and likely. Given that the discovery and transmission is easily possible, the real proof is that the Aboriginal lore gives an unambiguous statement that these stars do indeed vary in brightness, as collected by many ethnographers over a century ago from many Aboriginal groups. So I strongly conclude that the Aboriginal Australians could and did discover the variability of Betelgeuse, Aldebaran, and Antares.

physics.hist-ph↗

On the Observations of the Penetrating Radiation during Seven Balloon Flights

At the beginning of the twentieth century, the Austrian (later naturalized American) Victor Hess among others developed a brilliant line of research, leading to the final determination of the extraterrestrial origin of part of the atmospheric radiation. Before his work, the origin of the radiation today called "cosmic rays" was strongly debated, as many scientists thought that these particles came integrally from the crust of the Earth. There was however an active and rich research on the topic. Victor (at that time Viktor) Hess measured in 1912 the rate of discharge of an electroscope that flew aboard an atmospheric balloon. Since the discharge rate increased as the balloon flew at higher altitude, he concluded that the origin of part of the natural radiation could not be terrestrial. For this discovery, Hess was awarded the Nobel Prize in 1936, and his experiment became legendary. The fundamental article published by Victor Hess in 1912, reporting a significant increase of the radiation as altitude increases, is translated and commented here. The decisive measurement was performed in the last of the seven flights on aerostatic balloon described.

physics.hist-ph↗

Has CHSH-inequality any relation to EPR-argument?

We emphasize the role of the precise correlations loophole in attempting to connect the CHSH type inequalities with the EPR-argument. The possibility to test theories with hidden variables experimentally by using such inequalities is questioned. The role of the original Bell inequality is highlighted. The interpretation of the CHSH inequality in the spirit of Bohr, as a new test of incompatibility, is presented. The positions of Bohr, Einstein, Podolsky, Rosen, Bell, Clauser, Horne, Shimony, Holt, De Broglie, Hertz, and Boltzmann on interrelation of theory and experiment are enlightened.

quant-ph↗

Theoreticians at the Physical-Technical Institute (To the centennial of the Ioffe Institute)

Dedicated to the centenary of the Ioffe Institute, the article contains the shortest review of scientific achievements of the theorists of the institute during this time. We concentrate mainly on research in the field of elementary particle physics, astrophysics, nuclear theory and atoms. To obtain very important scientific results became possible because outstanding theoreticians worked at this Institute. The high level of research persisted in spite of several mass moves of theorists - then to Kharkov, then to Moscow, then abroad. The author can testify to the atmosphere that reigned in the FTI in person, since he works at this institute since 1958. The article deals not only with research activity, but also with the famous physics schools and their outstanding cultural programs. We present also examples of extraordinary successful activity of theorists far beyond the field of their narrow specialization.

physics.hist-ph↗

The Geometry of Spaceborne Synthetic Aperture Radar

The paper defines a new coordinate system that was developed in 1977-78 for the world's first digital synthetic aperture radar (SAR) ground processor for images from the Seasat-A satellite. The coordinate system is for the range-Doppler paradigm in the context of a spaceborne platform orbiting a rotating planet. The mathematical expressions for the azimuth FM rate, isodoppler lines, target illumination trajectories and antenna attitude determination from Doppler centroid measurements are derived. The method for transforming the SAR images from that SAR digital signal processor that used these parametric inputs is also presented. The paper concludes with a report of the measurement of the map accuracy of the resulting images.

physics.hist-ph↗