ASPACE-Q 

The Astrophysics,  Space  Exploration and Quantum Computing Group   

 ASPACE-Q 

The Astrophysics,  Space  Exploration and Quantum Computing Group   

by Valentin Cezar Ionescu

20.02.2026
















Credit: Educational representation of the Page–Wootters mechanism (Clock C and Rest R).

One of the most difficult questions in modern physics is surprisingly simple: does time exist as we perceive it? In everyday life, time seems obvious - the clock ticks, people age, things change. However, when we try to put together the two great theories of physics (quantum mechanics and general relativity), serious problems arise.

In quantum mechanics, the evolution of a system is described in time: the state changes as time passes. In general relativity, however, time is not a fixed background, but part of the geometry of the universe. In other words, time is no longer just an 'external clock' that flows the same everywhere. When physicists try to quantify gravity, a famous equation (Wheeler-DeWitt) emerges that, in its simplified form, seems to say that the overall state of the universe does not evolve at all. This has sometimes been called the 'frozen formalism': on a global scale, everything seems static, so there is no such thing as time.

But if the universe were globally 'static', how does the change we see occur? This is where the relational idea comes in: perhaps time is not something fundamental, but arises from the relationships between the parts of the system. More precisely, a subsystem can play the role of a clock, and the rest of the system is described in relation to it. So, instead of saying 'what happens at time t' in an absolute sense, we say 'what happens to the system when the clock shows a certain value' [2,4].

This idea was elegantly formulated by Page and Wootters. They propose a universe divided into two parts: a quantum clock (C) and the rest (R). The total state may be stationary (so, from the outside, nothing 'flows' in time), but between C and R there are quantum correlations (entanglement). When we condition the description of R on a certain 'reading' of the clock C, we get a sequence of states that looks exactly like an evolution in time. In short: time can arise from correlations, not necessarily from a fundamental external parameter [3].

The figure shows the central idea of the Page–Wootters mechanism: the total ensemble (Quantum Clock C + Rest R) can be described globally as stationary (without assuming a privileged external time), but for an internal observer using C as a reference, Rest R appears to evolve. This “evolution” is relational: it arises from the correlations (usually entanglement) between C and R and from the conditioning on a reading of the clock. Top (Quantum Clock C). Clock C is represented by a family of states denoted |t_C, which correspond to different “readings”. The “Time” axis suggests that these states can be ordered and used as internal labels t. Important: in this image, t is not an external time imposed on the universe, but a coordinate operationally defined by clock C. Center (Total Ensemble C + R and the Hamiltonian). The central box shows that the "universe" under consideration is bipartitioned into C (the clock) and R (the rest). In the simplified version in the figure, the total Hamiltonian is suggested as H = H_C + H_R. The pedagogical message: at the global level (C+R) we do not introduce from the start an evolution with respect to an external temporal parameter; instead, the relevant “time” will be that defined by the internal clock C. Left (Correlation between C and R). The bubble on the left emphasizes that C and R are not independent: correlations of the form |t_C |ψ(t)_R appear. Intuitively, for each possible reading of the clock C, the rest of R is associated with a corresponding state |ψ(t)_R. A schematic writing of the idea is that the global state can be seen as a superposition of such “correlated pairs”: |ΨΣ_t |t_C |ψ(t)_R (where the sum can also be an integral, as the case may be). Right (Conditional evolution of R). On the right is the key step: if we “fix” a clock reading (e.g., the clock indicates t), then the description of R becomes the conditional state obtained by projection onto C. The formula in the figure, t|_C |Ψ |ψ(t)_R, expresses just this. From the perspective of an internal observer using clock C, the dependence of R’s state on t is interpreted as the dynamics of R. Bottom (State sequence of R). The bottom colored bar represents the “movie” of R’s conditional states: at clock reading T0, R is in |ψ(T0)_R; at clock reading T1, R is in |ψ(T1)_R; at clock reading T2, R is in |ψ(T2)_R, etc. The visual conclusion is that an apparently temporal sequence of R’s states can arise from the correlation with C, even if the global description of the ensemble C+R is stationary.

An important point is that this idea did not remain only philosophical. Moreva et al[1] performed an experiment with two entangled photons to illustrate the Page-Wootters mechanism. One photon was treated as a 'clock', the other as a 'system'. Depending on how the experiment is viewed, two perspectives emerge: for an 'internal' observer, who uses one of the photons as a reference, the other appears to evolve; for a 'super-observer', who has access to the global properties of the pair, the total state remains practically unchanged.

The result is interesting because it operationally shows something profound: the same quantum reality can appear dynamic from the inside and static from the outside, without contradiction, if we take into account the role of correlations and the way in which we make the measurement. Moreover, extensions of the idea show that when the clock is imperfect (as all real clocks are), limitations and decoherence effects appear - that is, a decrease in the clarity of the observed evolution.

It is essential to be rigorous in our conclusions. The experiment does not 'solve' the problem of time in quantum gravity. It does not quantify gravity itself, and it does not reproduce the entire mathematical structure of quantized general relativity. What it does do, however, is very valuable: it provides a laboratory demonstration that the idea of time emerging from quantum correlations is coherent and can be tested in controlled systems.

Perhaps time, as we experience it, is not a fundamental component of the universe, but a phenomenon that arises from the way in which the parts of the universe relate to each other. It is a radical but perfectly legitimate idea in modern physics, and one of the ways in which researchers are trying to understand how quantum mechanics and gravity fit together. In the long run, such ideas are relevant to very big questions: what happens near black holes, how we describe the very early universe, and what a complete theory of quantum gravity would look like. Even though the photon experiment is simplified compared to the real universe, it has enormous value as a conceptual model: it shows that our intuitions about time can be tested step by step, not just discussed abstractly.

References:

[1] E. Moreva et al., „Time from quantum entanglement: an experimental illustration”, arXiv:1310.4691 (2013); Phys. Rev. A 89, 052122 (2014).

[2] B. S. DeWitt, „Quantum Theory of Gravity. I. The Canonical Theory”, Phys. Rev. 160, 1113–1148 (1967).

[3] D. N. Page, W. K. Wootters, „Evolution without evolution: Dynamics described by stationary observables”, Phys. Rev. D 27, 2885 (1983).

[4] K. V. Kuchař, „Time and interpretations of quantum gravity”, în: Proceedings of the 4th Canadian Conference on General Relativity and Relativistic Astrophysics, ed. G. Kunstatter, D. Vincent, J. Williams (World Scientific, Singapore, 1992).



by Dr. Alice Mihaela Păun

28.12.2025


















Courtesy: CXC/M Weiss

Dark Matter is the invisible material that makes up about 85% of all matter in the Universe. For a long time, researchers have been trying to provide an answer to this question: What is Dark Matter made of?

A new theoretical proposal is that Dark Matter could actually be something very strange: nuggets of Strange Quark Matter. This is the most extreme form of matter, an extremely dense “soup” made of three types of fundamental particles called quarks (up, down, and strange quarks). According to several theoreticians like Witten, De Rujula, Di Clemente et al., strange quark matter could have been formed shortly after the primordial explosion (Big Bang), a period of time in which the Universe was very young, hot, and chaotic. I the conditions were right, small, very dense aggregates made of this material could have formed and survived as relics up to this date, floating through space as Dark Matter.

An even more interesting fact is that the strange quark matter may be more stable than ordinary matter. If this is true, the consequences would entirely change everything we know about physics. Common matter like iron would not be the ultimate ground state of nature anymore, but instead a tightly packed mixture of up, down, and strange quarks, denser than anything we can create on Earth, would take its place.

Moreover, a study by astrophysicist Fridolin Weber shows that if strange quark matter really is stable, then some neutron stars, already among the densest objects in the cosmos, may actually be something even more extreme: Strange Quark Stars. These exotic stars would be made almost entirely of quark matter and could spin faster, shine differently, and behave in ways unlike ordinary neutron stars. If dark matter is made of strange quark matter, scientists argue that strange quark stars should certainly exist. Over billions of years ago, tiny dark matter “seeds” could collide with dense stellar cores, triggering several transformations inside stars and converting them into quark stars.

The first question that pops into everyone’s mind: why haven’t we seen strange matter yet? The answer is short and elusive: Strange quark matter would be extremely rare and heavy, and mostly…invisible, just like Dark Matter. New generations of neutrino telescopes, gravitational wave detectors, and space telescopes are continuously developing, so scientists may soon be able to test whether the Universe is filled with this exotic form of matter and whether some stars have already crossed the line into the unknown.

References:

1.    E. Witten (1984) Cosmic separation of phases. Physical Review D 30, 272-285, https://doi.org/10.1103/PhysRevD.30.272

2.    A. De Rujula, S. L. Glashow (1984) Nuclearites – a novel form of cosmic radiation. Letters to Nature 312, 734–737, https://doi.org/10.1038/312734a0

3.    Weber, F. (2016). Strange Quark Matter Inside Neutron Stars. In: Alsabti, A., Murdin, P. (eds) Handbook of Supernovae. Springer, Cham. https://doi.org/10.1007/978-3-319-20794-0_71-1

4.    Di Clemente, Francesco & Casolino, Marco & Lattanzi, Massimiliano & Ratti, Claudia. (2025). Strange quark matter as dark matter: 40 years later, a reappraisal. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1093/mnras/staf087

by Ph.D. student Andreea Monica Scorța

12.12.2025

















Credit: NASA: An artist's concept of the ESA-NASA SOHO spacecraft

Since the launch of the ESA/NASA Solar and Heliospheric Observatory (SOHO) on 2 December 1995, the supposedly only two-year mission, is still providing continuous news on the Sun’s activity. 

SOHO Mission carries on with what it was designed for: the characterisation of the solar seismology, visible surface, corona and the origin of the solar wind, thus helping the scientists better understand the Star that literally our world is orbiting around, but also opening the doors to “more discoveries, including more than 5,000 comets” (making it more than half of all known comets). [https://science.nasa.gov/mission/soho/]












Credit: https://en.wikipedia.org/wiki/Solar_and_Heliospheric_Observatory


It is quite impressive how the discovery of the comets was possible. One specific instrument on board SOHO, the Large Angle and Spectrometric Coronograph (LASCO) handle the brightness of the photosphere, by using a solid, internal disc called an <<occulter>> to block out the direct light from the Sun, creating a permanent, artificial eclipse of the instrument. In this manner, LASCO can focus on the extremely faint light scattered by the plasma and dust in the surrounding corona. The comets that pass too close to the Sun to be seen by other telescopes, are detected by the high-contrast field of view of LASCO.











Credit: https://lasco-www.nrl.navy.mil/index.php?p=content/intro#:~:text=A%20coronagraph%20is%20a%20special,as%20the%20%22corona%22)

Of course, this instrument achieved something unexpected and what it was not thought of it can do, but also, fulfilled the initial aim, the one of characterization of Coronal Mass Ejections (CMEs). 













Credit:SOHO's 30 years in numbers.

SOHO is a longaeval mission, that covered two 11-years full solar cycles up until now. This joint ESA-NASA projects have brought its contribution to the International Solar-Terrestrial Physics Programme, having more than 1500 scientists from around the world working on its data and it provides guidelines for the next generation of solar observatories, in terms of technology and science.













Credit: 30 years of SOHO imaging the Sun 


References:

https://www.esa.int/Science_Exploration/Space_Science/SOHO/Sun-watcher_SOHO_celebrates_thirty_years

https://www.esa.int/Science_Exploration/Space_Science/SOHO_overview

https://lasco-www.nrl.navy.mil/index.php?p=content/intro#:~:text=A%20coronagraph%20is%20a%20special,as%20the%20%22corona%22

https://science.nasa.gov/mission/soho/

by Andrei Militaru

05.12.2025














Credit: https://scitechdaily.com/revealed-first-dormant-stellar-mass-black-hole-in-our-cosmic-backyard/

Black holes are usually discovered using the radio and x-ray emission of the surrounding accretion disk, but a new type has been recently discovered thanks to new methods of detection. 

Those have being named dormant black holes with luminous companions, and 3 such black holes have been discovered by the mission Gaia: Gaia BH1, BH2 and BH3, with Gaia BH1 being the closest discovered black hole to our Solar system, at a distance of 1560 light years away. 

Researchers at Xinjiang University compared 2 evolution models to find which reflects the observations of dormant black hole systems better. The first model starts from an isolated binary star system, while the second starts with a triple star system. Their study concludes that triple star system in which the inner binary stars collapsed into a black hole may be the most common way dormant balck hole systems have been created.

Source: https://arxiv.org/pdf/2512.04774

by Florin-Ioan Constantin, Ph.D. student

07.11.2025














Simulation of a TDE, Source: Price et al. (2024) https://iopscience.iop.org/article/10.3847/2041-8213/ad6862


This week, a team of researchers published a study about one of the brightest events ever recorded.

In 2018, a flare was observed originating from a supermassive black hole located at the center of a galaxy 11 billion light-years away. The event was the brightest of this type ever recorded, with an intensity 10 trillion times greater than that of the Sun at its peak. After this spectacular maximum, the flare remained visible even as it "faded" over the course of 6 years of subsequent observations. Calculations show that the energy emitted...

In the article published in the journalNature, the research team proposes several theories about the source of the event, highlighting the one considered to be the most probable, namely that the black hole "tore apart" a star at least 30 times larger than our Sun located in the accretion disk of the black hole and which approached it too closely, in an event called a ‘tidal disruption event’.

The researchers also say that there are indications that such events could happen more often in the future, allowing them to learn more about the mechanisms that drive the accretion processes of supermassive black holes in the center of galaxies.

References:

https://www.nature.com/articles/s41550-025-02699-0#Sec5

https://www.nature.com/articles/d41586-025-03597-1

https://www.reuters.com/science/star-eating-black-hole-unleashes-record-setting-energetic-flare-2025-11-04/


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