DE / EN
2020/2021
History and Philosophy of Physics Research Seminar (Summer)

Time and Place:
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Tuesdays from 16:15 to 17:45 CEST.
Online via Zoom.
Zoom-links and weekly reminders are announced via hpp@listen.uni-bonn.de. Subscribing to this list is possible a) here, b) by sending an empty email to hpp-subscribe@listen.uni-bonn.de, or c) by contacting nmartens[at]uni-bonn[dot]de
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Conveners:
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Prof. Dr. Dennis Lehmkuhl & Dr. Niels Martens
13 April 2021
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Martin Lesourd (Black Hole Initiative, Harvard & Clark University)

What can observers know about their spacetime?

In general relativity (Lorentzian geometry more precisely), one can make this question mathematically precise and study it rigorously. J.Earman, C.Glymour, D.Malament, JB Manchak have all contributed to the question. The most up to date results (before this work) are due to JB Manchak and these seem to suggest a strong sense of epistemic underdetermination, i.e., the answer to the question being `global facts about our spacetime are out of reach in a strong sense' . I'll describe some new results that shed new light on this and I'll state some attractive open questions. 
20 April 2021
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Adam Koberinski (University of Waterloo & University of Bonn)

How effective is inflation?

Inflation is currently a key component of the cosmological model of the early universe. First developed to solve the horizon and flatness problems, its empirical success in predicting the scale-invariant spectrum of inhomogeneities in the cosmic microwave background has cemented inflation as a major component of our understanding of the universe. Standard accounts of inflation involve a scalar field driving exponential expansion of the universe. Coupled with an understanding of our best quantum field theories as effective field theories, many physicists (Weinberg 2008, Cheng et al. 2008) take inflation to be an effective field theory as well.
 
In this talk I will distinguish two notions of effective field theory that are often conflated. The former, loose sense of effective is that the theory is approximate and taken to only be valid in a limited domain, while the second employs the full machinery of the renormalization group, scale separation, and allows one to place quantitative error bounds on calculations made with the theory. I argue that, while inflationꟷalong with many other theoriesꟷis effective in the first sense, it is not in the more robust sense. This has implications for the extent to which we can think of inflation “washing away” the physics of the early universe. If inflation is not an effective field theory in the latter sense, then it is currently a (highly successful) phenomenological model that faces major foundational hurdles to being a useful guide for further inquiry into the early universe. I will end by discussing implications of the argument for exploring alternatives to inflation. In particular, one should prioritize approaches that lead to a fruitful enterprise of early universe cosmology; deviations from the expected behaviour point the way to new physical features relevant to the domain.
27  April 2021
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Shannon Sylvie Abelson (Indiana University, Bloomington)

The fate of TeVeS

The GW 170817 event co-detected by the LIGO and Virgo observatories registered simultaneous arrival times for gravitational waves and electromagnetic radiation emanating from a binary star merger. This detection event has been treated consistently within recent literature (Boran, et al. 2018; Green, et al. 2018; Baker, et al. 2017; Sakstein and Jain 2017; Schmidt 2017) as a crucial test of all alternative theories of gravity which postulate gravitational waves propagate along separate geodesics from electromagnetic spectra—a test such theories fail. These theories are purportedly thereby falsified. This includes relativistic extensions of Milgrom’s Modified Newtonian Dynamics (MOND), perhaps most notably Bekenstein’s Tensor-Vector-Scalar gravity (TeVeS). I critically examine the explicit endorsement of this case as one of falsification by members of the scientific community. While the current state of these theories is dim, it is not clear that recent developments in multimessenger observation can supply a decisive falsification. Rather this evidence should be regarded as merely disconfirmatory. The recommendation of caution regarding philosophical terminology in this case is intended to underscore the importance of having a consistent testing and confirmation methodology. The reliance upon over-simplified historical views from the philosophy of science is likely to be more of a hindrance than a help. 
4 May 2021
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Noah Stemeroff (University of Bonn)

Weyl on the methodology of physical inquiry (or why we can't teach theoretical physics to babies, no matter what Chris Ferrie says)

There is a common belief concerning the nature of scientific knowledge, which suggests that successful physical theories provide an accurate picture of reality. To understand a theory, we simply need to understand this picture and what it says about the world. Against this belief stands the idealist tradition in the philosophy of science, which suggests that the distinction between ‘theory’ and ‘reality’ is untenable. To the idealist, ‘reality’ is, at least in part, a theoretical construction. In this talk, I will provide an introduction to Weyl's idealism and the ‘mathematics-dictates-physics’ methodology it supports. In particular, I will focus on Weyl’s account of the role that both history and philosophy play in securing a mathematical harmony in the theoretical construction of reality, and the challenge this account poses to traditional scientific realism. At some point, I will also clarify what all this has to do with the burgeoning theoretical physics for babies literature.
11 May 2021
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Debate: The Merits of Semi-Classical Gravity

Erik Curiel (Munich Center for Mathematical Philosophy & Black Hole Initiative)
Christian Wüthrich (University of Geneva)
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18 May 2021
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Anna Ijjas (Max Planck Institute for Gravitational Physics)

A new kind of cyclic universe

In this talk, I will discuss how combining intervals of ultra-slow contraction with a (non-singular) classical bounce naturally leads to a novel cyclic theory of the universe in which the Hubble parameter, energy density and temperature oscillate periodically, but the scale factor grows by an exponential factor from one cycle to the next. 
BREAK
1 June 2021
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Robert Rynasiewicz (Johns Hopkins University)

How not to argue that distant simultaneity is conventional

In 1905 Einstein averred that the one-way speed of light in vacuo, and thus the simultaneity of distant events, is a matter of convention. Setting that speed to c in all directions, the principle of relativity together with the light postulate entails that judgments of simultaneity are relative to the choice inertial frames. Reichenbach showed in the early 1920's that the latitude in the original choice of a simultaneity criterion corresponds to the freedom in the choice the parameter ε anywhere between 0 and 1 (exclusively) in the equation

                                             t2 = t1 + ε(t3 – t1)

wherein t1 is the time of departure from point A, t2 the time of arrival and reflection at point B, and t3 the time of return to point A. Subsequently, Grünbaum saw this as defining the region of "topological" simultaneity between future and past light cones, which indicated to him that there is no causally definable hyperplane of simultaneity through their point of intersection. However, Malament showed in 1977 that this is mistaken: the plane that is Minkowski orthogonal to the observer's world line is picked out by causal criteria alone. On this ground, Malament went on to conclude that the criterion for frame relative simultaneity is not conventional.

In this talk, I argue that Grünbaum simply missed Einstein's point. It was for that reason that Malament was able to produce a result in conflict with Grünbaum's contention. But Malament also missed the point, leading him to the false conclusion that frame-relative simultaneity is not conventional. I go on to suggest that in the current divide on the topic, those in the non-conventional camp are typically confused with Grünbaum and Malament on what's at stake in the debate.
8 June 2021
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​Richard Staley (University of Cambridge)

The epistemologist and the history of relational mechanics: Mach, Einstein, Rovelli

Mach’s major contributions to the development of relativity have long seemed to be primarily epistemological - as Einstein avers in his well-known obituary, for example. This paper examines the origins of much of Mach’s work in psychophysics in the 1860s and 70s and his own account of the nature of epistemology from the 1890s onwards to argue instead for a more fluid approach to what has counted as ‘science’ and ‘epistemology’ at different times, while exploring different moments in the history of relational mechanics in the work of Mach, Einstein and Carlo Rovelli.
15 June 2021
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Tiffany Nichols (Harvard University, Dept. of the History of Science & Black Hole Initiative)

The Blueberry Barrens as a Potential Site of Gravitational Wave Detection: Early Understandings of the Role of Land in the Detection of Gravitational Waves

Current literature has unduly collapsed the site selection history of the Laser Gravitational Wave Observatory (LIGO) to a claimed U.S. Congressional decision for LIGO's sites.  My research reveals that the site selection history is more expansive.  By providing an account of LIGO's holistic site selection history, my research shows the importance of land considerations in gravitational wave detection.  This talk will focus on LIGO physicists' initial consideration of a site in the blueberry barrens of Maine during the 1980s.  I will discuss how land features, geological history, and social characteristics of the land became features of the experiment and quest to detect gravitational waves.
22 June 2021
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Kevin Coffey (NYU Abu Dhabi)

Symmetry and Interpretation in Newtonian Gravitation

It has long been recognized that Newtonian gravitation theory exhibits an important symmetry with respect to its inertial structure. Many philosophers of physics have used this fact to conclude that inertial structure within the theory ought to be interpreted as a gauge quantity—a conventional choice without underlying physical significance. This claim originally took shape in the cosmological context, but has now been extended to all models of Newtonian gravitation. In recent years, this argument has also played a role in attempts to show that Newtonian gravitation theory is theoretically equivalent to Newton-Cartan theory, a ‘geometrized’ counterpart to Newtonian gravitation. In my talk I aim to challenge this interpretation of Newtonian gravitation: despite the noted symmetry, I’ll argue that there are good reasons not to interpret its inertial structure as a gauge quantity. In the process, I hope to reveal an unappreciated aspect of the relationship between symmetries and theory interpretation.
29 June 2021
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William L. Vanderburgh (California State University, San Bernardino)

What We Don't Know Could Fill the Universe–And It Does

Given the fact that we have known about the dark matter problem since at least Zwicky 1933, it is rather surprising that we don't yet have a good idea what its solution is. This is even more surprising if you read the popular science press since, dozens of times in recent decades, they have announced that the dark matter mystery has been "solved." Every good idea seems to be quickly shot down and we are left with little but uncertainty. In my talk for the Philosophy of Dark Matter Workshop earlier this spring, I argued that Multi-messenger Astronomy is a model for how we could come to know enough to be scientific realists about dark matter. This paper builds on that one by looking for specific detailed examples of multiple measurement, consilience, multimodal evidence and related evidential concepts in the search for dark matter. It concludes that while there are prospects for fulfilling our hope to discover the nature of dark matter and confirm its role in astrophysics and cosmology, it is still possible that we may never achieve this hope. At this point, we need to wrestle with the possibilities that (1) even if have good reason to think that dark matter exists, it may be a kind of stuff it will be impossible for us ever know and that (2) pursuing knowledge of dark matter might not be worthwhile from the point of view of the costs in time, talent, resources, and lost opportunities to study other things.
6 July 2021
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Panel: Epistemology of Very Large Experiments

Event Horizon Telescope
Jamee Elder (Black Hole Initiative, Harvard & University of Bonn)
Juliusz Doboszewski (University of Bonn & Black Hole Initiative)

LIGO-Virgo 
Jamee Elder (Black Hole Initiative, Harvard & University of Bonn)
Lydia Patton (Virginia Tech)

Large Hadron Collider
Christian Zeitnitz (University of Wuppertal)
Florian Boge (University of Wuppertal)
13 July 2021
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Jeremy Butterfield & Henrique Gomes (University of Cambridge)

​A Noether Hole Argument

​The infamous hole argument---devised by Einstein and revived by Earman & Norton (1987)---has recently found its third wind. The spark that ignited yet another round of debate was Weatherall (2018)'s claim that proper attention to the mathematical structure of general relativity sufficed to disarm the indeterminism implied by the hole argument. One of Weatherall (2018)'s main ideas is to stipulate that, under the right notion of model-isomorphism, points of the manifold necessarily get dragged along with the metric.

While cousins of this reply have appeared in several different attempts to block the indeterminism, we will argue that it cannot encompass all there is to the concept of diffeomorphism symmetry in general relativity. For, by dragging metric and spacetime points together, the effects of a diffeomorphism operation are, in a sense, trivialized. As a result, any idea of symmetry that is associated with this operation cannot secure conservation laws.

The upshot will be that general relativity uses, and needs to use, two distinct notions of identification for the points in the underlying manifolds of symmetry-related models: a notion using a diffeomorphism to drag the metric; and a contrasting notion that individuates spacetime points independently of their metrical relations. But only the latter is non-trivial, in a sense that we describe.
20 July 2021
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Frank Bertoldi (University of Bonn)

Title tba
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Philosophy of Lambda Workshop
This online workshop focuses on various philosophical aspects of Lambda, i.e. dark energy/ the cosmological constant/ vacuum energy. Nora Mills Boyd and Genco Guralp will discuss experimental aspects. Adam Koberinski, Mike Schneider and David Wallace will debate the cosmological constant problem. ​The workshop will take place on Wednesday the 16th of June 2021, via Zoom. If you are already signed up for the hpp@listen.uni-bonn.de mailing list, there is no need to register for the workshop; you will receive the Zoom-link via the mailing list roughly one week before the workshop. If not, please register via this form. If you have any questions, please contact the organisers: Juliusz Doboszewski (jdobosze[at]uni-bonn.de) and Niels Martens (nmartens[at]uni-bonn.de).

All times below are in CEST. During the breaks it will be possible to informally chat with the speakers and other participants via the platform Wonder; a link will be sent out in due course.​
14:30-15:30
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Nora Mills Boyd (Siena College)

Do's and Don'ts from DES: Epistemic challenges in combining constraints from multiple dark energy probes
Break (15 min)
15:45-16:45
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Genco Guralp (San Diego State University)

Dark Energy Measurements with Type Ia Supernovae: Mapping the Systematic Uncertainty Terrain
Break (15 min)
17:00-19:00
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Debate - The Cosmological Constant Problem

Adam Koberinski (University of Waterloo & University of Bonn)
Mike Schneider (University of Pittsburgh)
David Wallace (University of Pittsburgh)
Philosophy of Dark Matter Workshop
This online workshop is being organised as part of the project "LHC, dark matter & gravity", and will take place on 29-30 March 2021 via Zoom. Click here for further info, incl. (free) registration. The times in the schedule below are in CEST.
History and Philosophy of Physics Research Seminar (Winter)

Time and Place:
Tuesdays from 16:15 to 17:45 CET.
Online via Zoom.
Zoom-links and weekly reminders are announced via hpp@listen.uni-bonn.de; contact nmartens[at]uni-bonn[dot]de to be added to this mailing list.
3 Nov 2020
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Juliusz Doboszewski (University of Bonn)

Kerr black holes as time machines

Spinning black holes are now considered to be a well-established feature of our universe. However, some maximal extensions of certain spinning black hole spacetimes (such as the Kerr spacetime) have chronology violating regions. How likely is it, then, that our universe contains chronology violating regions? In this talk, I will discuss whether and to what extent spinning black hole spacetimes could be seen as a time machine in some precise sense, and critically assess a recent claim that time machines (and other forms of time travel to the past in general relativity) are incompatible with the second law of thermodynamics.
10 Nov 2020
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Richard Dawid (Stockholm University)
Based on joint work with Casey McCoy (Yonsei University)

How postmodern is cosmic inflation?
 
In 2014, Ijjas, Loeb and Steinhardt (ILS) claimed that the paradigm of eternal inflation had left the regime of canonical scientific reasoning (using the pejorative term postmodern inflation). The debate on their paper eventually led to a highly antagonistic and much publicized exchange between ILS and 40 main exponents of inflation in Scientific American. In my talk I will argue that the irreconcilable positions in this debate have genuine philosophical roots. I will sketch a Bayesian analysis of the problem raised by ILS and will argue that acknowledging the role of meta-empirical theory assessment is helpful for identifying the core of the disagreement.
17 Nov 2020
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Romain Ruzziconi (TU Wien)
 
Asymptotic symmetries in gravity and the BMS group in (A)dS           

I will start this talk by reviewing some aspects of asymptotic symmetries in gauge theories with a focus on General Relativity. I will insist on the deep implications of imposing boundary conditions for the general covariance principle. I will then introduce the notion of asymptotically flat spacetime and define the Bondi-van der Burg-Metzner-Sachs (BMS) group and its various extensions. Afterwards, I will propose a new definition of asymptotically (anti-)de Sitter ((A)dS) spacetime and show that the associated asymptotic symmetry group, called the Λ-BMS group, reduces to one of the extensions of the BMS group in the flat limit. Using the holographic renormalization procedure and a diffeomorphism between Bondi and Fefferman-Graham gauges, I will show that the flat limit is also valid at the level of the phase space.           

Based on: 1905.00971, 1910.08367, 2004.10769.
24 Nov 2020
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Joshua Eisenthal (Caltech & University of Bonn)
 
Hertz’s Mechanics and a unitary notion of force

Heinrich Hertz dedicated the last four years of his life to a systematic reformulation of mechanics. One of the main issues that troubled Hertz in the traditional formulation was a ‘logical obscurity’ in the notion of force. However, it is unclear what this logical obscurity was, hence it is unclear how Hertz took himself to have avoided this obscurity in his own formulation of mechanics.         

In this paper I will first identify an issue concerning the Newtonian conception of force that lay in the background of Hertz’s concerns. I will argue that a subtle ambiguity in Newton’s original laws of motion led to the development of two different notions of force: a vectorial notion and a variational notion. I will then explore how Hertz employed the mathematical apparatus of differential geometry to arrive at a unitary notion of force, thus avoiding the logical obscurity that lurked in the traditional formulation of mechanics.
1 Dec 2020
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Emilie Skulberg (University of Cambridge)
 
Visual representations of the space around black holes         

The image of the shadow of a black hole released in April 2019 became an icon in the span of hours. Although this image was historic, if we consider visual representations such as visualisations from simulations, diagrams, and artist impressions, the iconography of black holes dates back decades before the release of imaging based on observation. The first part of my presentation provides a brief overview of this history. The second part accounts for the production of imaging within the Event Horizon Telescope Collaboration, which was behind the April 2019 image. The presentation is based primarily on fieldwork where I have studied the work of the collaboration, an analysis of their publications targeting various audiences, and the study of a collection of black hole imaging from 1973 to 2000. 
8 Dec 2020
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