Shot in the Dark

The Earth orbits the Sun at a brisk 107,000 km/hr (66,486 mi/hr). The Sun, in turn, circles the Milky Way at a staggering 828,000 km/hr (514,495 mi/hr). And deep in the galactic core, stars whirl around the supermassive black hole at relativistic speeds, up to 36 million km/hr (22,369,363 mi/hr). Gravity is the architect and master of this motion: the invisible hand that not only initiates these velocities but binds our galaxy into a luminous spiral of unity.

Except it shouldn’t. Not with the piddling amount of mass that we can see.

The Milky Way contains 60-100 billion solar masses, an impressive sum, but a puny, gravitationally insufficient amount. With only that amount of ordinary matter, the galaxy would disperse like dry leaves in a breeze. Its stars would drift apart, its spiral arms dissolve, and the universe itself would remain a diffuse fog of light and entropy, never coalescing into structure or verse. No Halley’s Comet. No seasons. No Vivaldi.

To hold the Milky Way together at its observed rotation speeds requires about 1.4 trillion solar masses, seven times the visible amount. And we know this mass is there not because we’ve seen it, but because the galaxy exists. Much like Descartes’ Cogito, ergo sum (“I think, therefore I am”), we reason: The Milky Way is; therefore, it must possess sufficient mass.

The problem is that 85% of that mass is missing; from view, from touch, from detection. Enter stage right: Dark Matter. It does not emit, absorb, or reflect light. It does not interact with ordinary matter in any known way. It is invisible, intangible, a Platonic ether of shadow reality. Without it, the sacrament of gravity and being floats away like a balloon on a huff and puff day. And the universe loses its meaning.

Much like the neutrino, predicted by theory, is a particle once postulated to preserve the sanctity of conservation laws, a piece of the quantum world long before it was ever seen. Dark Matter is another elusive phantom, inferred by effect, but physically undetected. Dark Matter bends light, sculpts galaxies, and governs gravitational dynamics, yet it inhabits a metaphysical realm that requires faith to make it real. Unlike the neutrino, it lacks a theoretical platform. The General Theory of Relativity insists it must have mass; the Standard Model offers it no space. It is an effect without a cause: a gravitational fingerprint without a hand.

Yet, physicists are trying to tease it out, not so much to grasp a formless ghost, but rather to catch a glimpse of a wisp, a figment, without knowing how or where to look. To bring light to the dark one must grope around for a switch that may or may not exist.

Researchers at the University of Zurich and the Hebrew University of Jerusalem have devised an experiment called QROCODILE: Quantum Resolution-Optimized Cryogenic Observatory for Dark matter Incident at Low Energy (One can only guess at the amount of time and gin the Docs spent on that acronym 😊) to help tease out the existence of Dark Matter.

The experiment is designed to detect postulated ultralight dark matter particles that may interact with ordinary matter in currently unfathomable ways. To find these particles they have built a detector of superconducting nanowire sensors, cooled to near absolute zero, that achieves an astounding sensitivity to detect an infinitesimally small mass of 0.11 electron-volts (eV).

0.11 eV is roughly the energy difference between two quantum states in a molecule. An imperceptible shiver in the bond between two hydrogen atoms: a mass so slight, it might provoke a murmur of dark matter itself.

Using this detector over a 400-hour run (16.66 days) the team recorded a handful of unexplained signals that are real but not necessarily dark matter. Eventually they hope to achieve detections that resolve directionality, helping distinguish dark matter from background noise. The next phase of the experiment: NILE QROCODILE, (groan*) will move the detectors underground to reduce cosmic interference.

QROCODILE is a shot in the dark. It’s an epistemological paradox: how do you build a detector for something you don’t understand? How, or why, do you build an energy detector for a substance, if it is indeed a substance, that doesn’t emit or absorb energy.

While dark matter is known through its gravitational pull, that detection at a particle level is infeasible. Energy detectors, then, are a complementary strategy, betting on weak or exotic interactions beyond gravity.

Whether it finds Dark Matter or not, QROCODILE reminds us that science begins not with certainty, but with the courage to ask questions in the dark, and the craftsmanship to build instruments that honor the unknown.

* NILE QROCODILE: an acronym that evokes remembrance of the socially awkward Dr. Brackish Okun, a secluded researcher of aliens and their tech at Area 51 in the 1996 movie Independence Day.

Source: …Dark Matter Search with QROCODILE… by Laura Baudis et al, Physical Review Letters, 2025. Graphic: Nile Crocodile Head by Leigh Bedford, 2009. Public Domain.

Cosmos of the Lonely

The universe keeps expanding. When researchers analyze data from the Hubble and James Webb telescopes, alongside a suite of other astronomical tools, they find that the recessional velocity of galaxies, the speed at which they appear to move away from the Earth, varies depending on what they measure.

If they calibrate distances deep into the cosmos using Cepheid variable stars, the expansion rate appears faster than when they use red giant stars or the Cosmic Microwave Background (CMB). This discrepancy, known as the Hubble tension, reveals a deeper mystery: different cosmic yardsticks yield different rates of expansion.

Yet despite the disagreement in values, all methods affirm the same truth: space is stretching…a lot…like a sheet pulled and stretched taut between Atlas’s burden and Hermes flight: a cosmos caught between gravitational pull and a mysterious push: Pushmi-Pullyu on a cosmic scale.

To understand why the cosmos resembles a sheet of rubber we need to travel back about 110 years and peer into the minds of those who first saw increasing separation as a universal law. These new architects of reality: Einstein, Friedmann, Lemaitre; who replaced Newton’s planetary, static models of the cosmos with a dynamic spacetime of bends, ripples, and persistent expansion.

After Einstein published his General Theory of Relativity in 1915, Russian physicist Alexander Friedmann’s analysis of his work showed that the universe could be expanding, and that Einstein’s equations could be used to calculate the rate. In 1927 Belgium priest and physicist Georges Lemaitre proposed that the expansion might be proportional to a galaxy’s velocity relative to its distance from Earth. By 1929, American astronomer Edwin Hubble expanded on Lemaitre’s work and published what became known as Hubble-Lemaitre law: galaxies are moving away from us at speeds proportional to their distance. The greater the distance the faster the speed.

A key feature of this law is the Hubble constant, the proportionality that links velocity and distance. Hubble’s initial estimate for this constant was whopping, and egregiously off, 500 kilometers per second per megaparsec (km/s/Mpc), but as measurements improved, it coalesced around a range between 67 and 73, with the most recent value at 70.4 km/s/Mpc, published by Freedman et al. in May 2025.

The Hubble constant is expressed in kilometers per second per megaparsec. The scale of these units is beyond human comprehension but let’s ground it to something manageable. A megaparsec is about 3.26 million light-years across, and the observable universe, though only 13.8 billion light-years old, has stretched to 46 billion light-years in radius, or 93 billion light-years in diameter, due to the expansion of space (see mind warping explanation below).  

To calculate the recessional velocity across this vast distance, we first convert 46 billion light-years into megaparsecs: which equates to 14,110 megaparsecs. Applying Hubble’s Law: 70 km/s/Mpc times 14,110 Mpc equals 987,700 km/s. This is the rate at which a galaxy 46 billion light-years away would be receding relative to another galaxy one megaparsec closer to Earth.

That’s more than three times the speed of light (299,792 km/sec) or Warp 3 plus in Star Trek parlance. Einstein said this was impossible but fortunately there is some nuance that keeps us in compliance with Special Relativity (or else the fines would be astronomical). This isn’t the speed of a galaxy moving through space, but the speed at which space between galaxies is expanding. Which, admittedly, is terribly confusing.

The speed of a galaxy, composed of matter, energy, and dark matter, must obey Einstein’s rules: gravity and Special Relativity. And one of the rules is that the speed of light is the cosmic speed limit, no one shall pass beyond this.

But space between the galaxies decides to emphasize the rules in a different order. The expansion of space is still governed by Einstein’s equations, just interpreted through the lens of spacetime geometry rather than the motion of objects. This geometry is shaped by, yet not reducible to, matter, energy, and dark matter.

Expansion is a feature of spacetime’s structure, not velocity in the usual sense, and thus isn’t bound by the speed of light. If space wants to expand, stretch, faster than a photon can travel, well so be it.

The space between galaxies is governed by dark energy and its enigmatic rules of geometry. Within galaxies, the rules are set by dark matter, and to a lesser extent by matter and energy, even though dark energy is likely present, its influence at galactic scales is minimal.

Note the use of the word scale here. Galaxies are gigantic, the Milky Way is 100,000-120,000 light-years in diameter. But compared to the universe at 93,000,000,000 light-years across, they’re puny. You would need 845,000 Milky Ways lined up edge-to-edge to span the known universe.

Estimates of the number of galaxies in the universe range from 100 billion to 2 trillion. So, at the scale of the universe, galaxies are mere pinpoints of light; blips of energy scattered across the ever-expanding heavens.

This brings us to dark energy, the mysterious force driving cosmic expansion. No one knows what it is, but perhaps empty space and dark energy are the same. There’s even some speculation, mostly mine, that dark energy is a phase shift of dark matter. A shift in state. A triptych move from Newtonian physics to Quantum Mechanics to…Space Truckin’.

In the beginning moments after the big bang, the universe was dominated by radiation composed of high energy particles and photons. As the universe cooled, the radiation gave way to matter and dark matter. As more time allowed gravity to create structures, black holes emerged and a new force began to dominate, dark energy. But where did the dark energy come from? Was it always part of the universe or did it evolve from other building blocks. Below are a few speculative ideas floating around the cosmic playroom.

J.S. Farnes proposed a unifying theory where dark matter and dark energy are aspects of a single negative mass fluid. This fluid could flatten galaxy rotation curves and drive cosmic expansion, mimicking both phenomena simultaneously.

Mathematicians Tian Ma and Shouhong Wang developed a unified theory that alters Einstein’s field equations to account for a new scalar potential field. Their model suggests that energy and momentum conservation only holds when normal matter, dark matter, and dark energy are considered together.

Ding-Yu Chung proposed a model where dark energy, dark matter, and baryonic matter emerge from a dual universe structure involving positive and negative mass domains. These domains oscillate and transmute across dimensions.

These ideas all rotate around the idea that reality revolves around a concept that everything evolves and that matter and energy, of all forms, flickers in and out of existence depending on dimensional scaffolding of space and the strength of gravity and radiation fields.  Rather than radiation, energy, matter, dark matter, and dark energy as separate entities, these may be expressions of a single evolving field, shaped by phase transitions, scalar dynamics, or symmetry breaking.

Now back to my regularly scheduled program. In August 2025, Quanta Magazine reported on a study led by Nobel laureate Adam Riess using the James Webb Telescope (JWST) to measure over 1,000 Cepheid variable stars with unprecedented precision. Cepheid stars pulsate in brightness over time with a highly predictable rate or rhythm, making them ideal cosmic yardsticks. Riess’s team found a Hubble constant of ~73.4 km/s/Mpc, consistent with previous Hubble Space Telescope measurements of Cepheid stars but still significantly higher than what theory predicts.

That theory comes from the standard model of cosmology: Lambda Cold Dark Matter. According to this framework photons decoupled from the hot electron-proton opaque soup about 380,000 years after the Big Bang went boom, allowing light to travel freely for the first time, and allowing space to be somewhat transparent and visible. This event produced the Cosmic Microwave Background (CMB).

This CMB permeates the universe to this day. It was discovered in 1964 by Bell Lab physicists Arno Penzias and Robert Wilson, who were trying to eliminate background noise from their radio antenna. The noise turned out to be the faint afterglow from the Big Bang, cooled down from its original 3000 Kelvin to a frosty 2.7 Kelvin. They received the Nobel Prize in Physics for this discovery in 1978.

Light from the CMB, as measured by the European Space Agency Planck satellite, has a redshift of approximately 1100, meaning the universe has expanded by a factor of 1100 over the past 13.42 billion years. By analyzing the minute temperature fluctuations in the CMB, Planck can infer the density of matter, dark energy, and curvature of the universe. Inserting these parameters into the Lambda Cold Dark Matter model yields a Hubble constant which turns out to be 67.4 + 1.71 (65.69-69.11). This value is considered the gold standard. Values beyond the Planck measurement are not necessarily wrong, just not understood.

At first glance, the difference between Planck’s 67.4 and Riess’ 73.4 may seem small. But it is cosmically significant. Two galaxies 43 billion light-years away and 3.26 billion light-years apart (1000 Mpc) would have a velocity difference of 6000 km/s or about 189 billion kilometers of increased separation per year. That’s the scale of what small differences in the value can add up to and is referred to as the Hubble tension.

Meanwhile, a competing team of researchers studying red branch and giant branch stars consistently scored the Hubble constant closer to the theoretical prediction of 67.4. This team led by Wendy Freedman believes that Hubble tension, the inability of various methods of measuring the Hubble constant to collapse to a single value, is a result of measurement errors

While some researchers, Wendy Freedman and others, suggest lingering systematic errors may still be at play, the persistence of this discrepancy, across instruments, methods, and team, has led others to speculate about new physics. Among the most provocative ideas: the possibility that the universe’s expansion rate may vary depending on direction, hinting at anisotropic expansion and challenging the long-held assumption of cosmic isotropy. But this seems far-fetched and if true it would likely break the Lambda Cold Dark Matter model into pieces.

And so, the cosmos grows lonelier. Not because the galaxies are fleeing, but because space itself is stretching, a wedge governed by the geometry of expansion. The further they drift apart, the less they interact, a divorce from neglect rather than malice. In time, entire galaxies will slip beyond our cosmic horizon, receding faster than light, unreachable even in principle. A cosmos of the lonely.

Source: The Webb Telescope Further Deepens the Biggest Controversy in Cosmology by Liz Kruesi, Quanta Magazine, 13 August 2024. JWST Observations Reject Unrecognized Crowding of Cepheid Photometry as an Explanation for the Hubble Tension at 8σ Confidence by Riess et al, The Astrophysical Journal Letters, 6 February 2024. Graphic: Cosmic Nebula by Margarita Balashova.

Women and Glass: The Starlight Calculators of Harvard

In the halcyon days of yore before digital ubiquity and tonal exactitude, computers were made of flesh and blood, fallibility crossed with imaginative leaps of genius. Photographs etched starlight’s past onto glistening glass and preserved silver. Solid archives where memory endures and future discoveries shimmer with potential, encoded in celestial light of the heavens awaiting the discerning caress of curiosity, intuition, and reason.

In 1613, English poet Richard Brathwait, best remembered for his semi-autobiographical Drunken Barnaby’s Four Journeys, enshrined the word computer into written English while contemplating the divine order of the heavens, calling God the “Truest computer of Times.” Rooted in the Latin computare, meaning “to reckon together,” the term evolved over the next three centuries to describe human minds inimitably attuned to the interpretation of visual data: star fields, spectral lines, geologic cross-sections, meteorological charts, and other cognitive terranes steeped in mystery, teasing initiates with hints of vision and translation. These were not mere calculators nor unimaginative computers, but perceptive analysts, tracing patterns, exposing truths, and coaxing insights from fluid shapes etched into the fabric of nature.

By the time of the Enlightenment and the scientific revolution, human computers had become the invisible deciphering force behind truth seeking laboratories, the unsung partners in progress, cataloging, interpreting, and taming the flood of empirical but seemingly nonsensical data that overwhelmed those without insight. Harvard College Observatory was no exception. With photography now harnessed to astronomy’s telescopes, the observatory could suddenly capture and archive starlight onto glass plates of coated silver, forever changing astronomy from the sketches of Galileo to silver etches of eternal starlight.

But these glass plates, resplendent with cosmic information, remained galleries of dusty, exposed negatives, inert until absorbed and guided by human curiosity and insight.

Enter the women computers of Harvard, beginning in 1875, over 140 women, many recruited by Edward Charles Pickering, processed more than 550,000 photographic plates, the last collected in 1992, bringing much needed coherence and linearity to the chaos of too much. They sorted signal from celestial noise, revealing the hidden order of the universe inscribed in silver, preserved in silica.

In 1875 the initial cohorts, the pioneers, the first names of Harvard women computers, although not exactly given that moniker, to appear on the glass plates were names like Rebecca Titsworth Rogers, Rhoda G. Saunders, and Anna Winlock assisting in the absolutely essential process of what we would now call cross-referencing the glass plate’s ‘metadata’ with the astronomical data.  Ascertaining that time and space of the data match the time and space of the metadata. In 1881 Pickering, the observatory’s fourth director, began hiring women specifically as Astronomical Computers, a formal role focused on analyzing and deciphering the growing collection of glass plate photographs.

This shift in 1881 was more than semantic, a fancy title for drudge work and tedious plate cataloging but a structured program where women like Williamina Fleming, Annie Jump Cannon, Henrietta Swan Leavitt, and Cecilia Payne-Gaposchkin were tasked with not just cataloging stars, but studying stellar spectra, and the lights powering life and imagination throughout the universe. Indispensable efforts that lead to the Henry Draper Catalogue, eventually containing the half million plus glass plates, and the foundations of modern stellar classification systems and 21st century astronomy. Their stories are worthy of a Horatio Alger novel, maybe not exactly rags to riches, but certainly humble beginnings to astronomical fame. They were paid peanuts, but they were the elephants in the observatory.

Williamina Fleming, in 1879 arrived in Boston penniless and abandoned by her husband secured a job as a domestic in the home of Edward Pickering, yes that guy. She impressed Pickering’s wife, Elizabeth, with such intelligence that she recommended her for work in the observatory. She quickly outpaced her male counterparts and in 1881 was officially hired as one of the first Harvard Computers.

Studying the photographed spectra of stars, she developed a classification system, the natural human desire to find order in apparent chaos, based on the abundance of hydrogen on the surface of a star or more exact the strength of hydrogen absorption lines from the spectra data. The most abundant stars were classed as A stars, the next most abundant as B stars, and on down to V.

In 1896 Pickering hired Annie Jump Cannon, a physics degree from Wellesley and an amateur photographer, modified Fleming’s stellar classification system based also on the surface temperature of a star rather than hydrogen abundance. Her method was to use the strength of the Balmer absorption lines, electrons excited within hydrogen atoms, like dancers at different tempos, reveal themselves through subtle spectral lines now understood to be differing ionization states of the atom directly tied to the surface temperature of the star.

Her system used the same letters to avoid redoing the entire Harvard catalogue, but she reduced the list down to 7 and reordered them from hottest to coolest: O, B, A, F, G, K, M. Her classification is still in use today. Earth revolves around a G-class star which has a medium surface temperature of about 5800 K (9980 F or 5527 C).

Henrietta Swan Leavitt graduated from Harvard’s Women’s College in 1892 with what we might now call a liberal arts degree. A year later, she began graduate work in astronomy, foundation for employment at the Harvard Observatory. After several extended detours tucked under her petticoats, Edward Charles Pickering brought her back to the Observatory in 1903. She worked initially without pay, later earning an unfathomable 30 cents an hour.

There, Leavitt collaborated with Annie Jump Cannon, in a coincidence of some note both women were deaf, though one is left with the feeling that the absence of sound may have amplified the remaining sensory inputs to their fertile minds. In time, Leavitt uncovered a linear relationship between the period of Cepheid variable stars and their luminosity, a revelation that became an integral part of the cosmic yardstick for measuring galactic distances. The Period-Luminosity relation is now enshrined as Leavitt’s Law.

Cepheid variables form the second rung of the Cosmic Distance Ladder; after parallax, and before Type Ia supernovae, galaxy rotation curves, surface brightness fluctuations, and, finally, the ripples of Einsteinian gravitational waves. Leavitt’s metric would prove essential to Edwin Hubble’s demonstration that the universe is expanding.

Swedish mathematician Gösta Mittag-Leffler considered nominating her for the Nobel Prize in Physics, but his plans stalled upon learning she had died in 1921. The Nobel, then as now, is non-awardable to the dead.

Cecilia Payne-Gaposchkin, a transplanted Brit, joined the Harvard Observatory as an unpaid graduate fellow while working towards her PhD at Radcliffe in astronomy. Upon earning her doctorate, she continued at the Observatory with no title and little pay. By 1938 she was awarded the title of Astronomer and by 1956 was made full professor of Harvard’s faculty.

In her dissertation she accurately showed for the first time that stars are composed primarily of hydrogen and helium, proving that hydrogen was the most abundant element in the universe, overturning long held but erroneous assumptions. But in a twist of fate, astronomer Henry Norris Russell persuaded her to label her conclusions of hydrogen abundance as spurious. Four years later Russell’s research reached the same conclusion, but he barely gave her an honorable mention when he published his results.

She wasn’t the first nor will she be the last to suffer at the hands of egotistical professors, more enamored of self rather than truth, but her elemental abundance contribution to astronomy brushed away the conceit that stars must mimic rocky planets in their composition, much like Galileo ended Earth’s reign as a center of everything. Twentieth century astronomer Otto Struve hailed her dissertation as “the most brilliant PhD thesis ever written in astronomy.”

Undeterred and building on her studies of spectral emissions of stars she turned her gaze to high luminosity and variable stars with husband astronomer Sergi Illarionovich Gaposchkin. After 2 million observations of variable stars, their efforts laid the groundwork for stellar evolution: how stars change over the course of time. From hints of dispersed stardust to starlight and back again. Cycles of stellar life repeated billions of times over billions of years.

Harvard’s astronomical female human computers, initially mere clerks transcribing stars from silver and glass, evolved into interpreters of light, shaping the very foundations of astronomy. Through logic, imagination, and an unyielding devotion to truth, they charted the heavens and opened lighted pathways for generations to follow.

Graphic: The Harvard Computers standing in front of Building C at the Harvard College Observatory, 13 May 1913, Unknown author. Public Domain

Sunny Side Up: Gömböc, Bille, and the Geometry of Falling

In Shel Silverstein’s poem “Falling Up,” a child trips on his shoelace and soars skyward instead of tumbling down. A delightful inversion of reality, a child’s imagination conjuring tomorrow’s focus. In the world of mathematics and physics, a similar inversion has captivated minds for decades: can you design an object that always falls the same way, always sunny side up, no matter how it starts, like a cat landing on all fours.

In the realm of numbers and materials this is the problem of monostability: creating a shape that, when placed in any orientation, will always return to a single, stable resting position. It’s a deceptively simple question with grudgingly difficult solutions. And it has at least two very different answers.

The first answer to the cat landing on all fours came in 2006 with the discovery of the Gömböc, a smooth, convex, homogeneous shape that rights itself without any differential weighting or moving parts. Invented by Hungarians Gábor Domokos and Péter Várkonyi, the Gömböc, meaning “little sphere or roundy” in Hungarian, has only one stable and one unstable equilibrium point. No matter how you place it, it will wobble and roll until it settles in its preferred orientation.

The Gömböc is a triumph of pure geometry. It solves the monostability problem using only shape, no tricks, no hidden weights but some serious math. It’s been compared to a mathematical cat: always landing on its feet, a design with a natural convergence toward the domed asymmetry of tortoise shells, whose shapes nature may have unconsciously optimized for self-righting.

Although uses for Gömböc are still being explored, some have developed designs for passive orientation systems, and the name has been co-opted for a company that is building self-correcting cloud infrastructure.

The second answer came recently in June of this year, when Gergő Almádi, Robert Dawson, and Gábor Domokos, of Gomboc fame, constructed a monostable tetrahedron, a four-faced scalene or irregular polyhedron that always lands on the same face which they named Bille: “to tip or to tilt” in Hungarian. A solution to a decades-old conjecture by John Conway, a Princeton polymath professor, with a talent for finding tangible solutions to abstract problems.

In this case, unlike the geometric solution of the Gömböc, geometry enables self-righting only when paired with carefully engineered mass distribution: a lightweight carbon-fiber frame and a dense tungsten-carbide core, precisely positioned to shift the center of gravity into a narrow “loading zone.” It’s a hybrid of form and force, where the shape permits monostability, but the mass forces the issue.

Unlike the Gömböc, which might inspire real-world designs, the monostable tetrahedron is too fragile, too constrained, and too dependent on ideal conditions to be practical. It’s a mathematical curiosity, not an engineering breakthrough. But like numerous mathematical solutions, practicality may occupy some interesting spaces in the future because landing on your feet is a useful function in many areas of commerce and science.

In space exploration lunar landers have recently had a bad, and expensive habit of falling over. In marine safety, users of escape pods and lifeboats prefer them to remain upright and watertight. Come to think most occupants of any watercraft prefer to remain upright and dry. Robots and drones benefit from shapes that naturally return them to a functional position without motors or sensors.

In the end, both the Gömböc and the weighted tetrahedron are about their inevitable position and stability. They are objects that always know where they stand. One does it with elegance; the other with abstraction and compromise. One is a cat. The other is a clever box of lead and air.

And maybe that’s the real lesson of “falling up”: that sometimes, the most interesting ideas aren’t the ones that solve problems, but the ones that reframe the question, and quietly remind us that some problems, left alone, reveal their own solutions.

As Calvin Coolidge once observed, “If you see ten troubles coming down the road, you can be sure that nine will run into the ditch before they reach you.” Meaning he didn’t need to attack and solve 10 problems, just the persistent one. The Gömböc and Bille didn’t wait for the problem to develop, they honored the ditch. Their designs never left the ditch. The problem never materialized in the first place.

Source: Mon-monstatic Bodies by Varkonyi and Domokos, Springer Science, 2006. Bulilding a Monostable Tetrahedron by Almadi et al, arXiv, 2025.

Life, the Universe, and Everything: Speculative Musings on the Cutting Edge of Physics

The Higgs boson, theorized in the 1960s, is a massive quantum particle central to the Standard Model of particle physics. It arises from the Higgs field, an invisible sea permeating all of space, which gives fundamental particles, like electrons and quarks, their mass. Unlike electromagnetic fields, created by moving charges like protons, the Higgs field exists everywhere, quietly shaping the universe. In 2012, CERN’s Large Hadron Collider detected the Higgs boson, confirming the field’s existence. While the boson is observable, the field remains invisible, known only by its effects on particle masses.

The Higgs field assigns mass, but gravity governs how that mass behaves across the vast scales of spacetime. Blending gravity with quantum mechanics, which includes the Higgs field, requires a yet-undiscovered theory of quantum gravity. If successful, quantum gravity might untangle physics-defying singularities, points of extreme density, into structured, comprehensible forms. Some theorize it could also reveal how early radiation morphed into matter, possibly influencing the formation and behavior of mysterious dark matter and its potential link to dark energy.

Before the Big Bang, some picture a singularity, a point of extreme density, though not necessarily infinite matter, where known physics and spacetime break down. Quantum gravity, however, hints this wasn’t truly infinite but a transition phase. From what? Perhaps a prior universe or a chaotic quantum state, science doesn’t yet know. This shift, possibly tied to the Higgs field, may have sparked quantum fluctuations, birthing radiation, matter, and the cosmic structure we see today.

What if the universe is cyclic, not a one-time burst? Instead of a singular Big Bang, some speculate a “bounce”, a transition where spacetime contracts, then expands again. Early on, energetic radiation like photons cooled and condensed into heavy particles, or fermions, a million times heftier than electrons. Some theorize these fermions underwent chiral symmetry breaking, like a spinning top wobbling one way instead of both, potentially forming cold dark matter, though evidence is sparse. This invisible web of dark matter stabilized galaxies, keeping them from spinning apart.

The Higgs field might have shaped dark matter by influencing the mass of early fermions, but this link is speculative, lacking direct proof. Dark matter, in turn, may be evolving. If it slowly decays or transitions into dark energy, as some hypothesize, it could drive the universe’s accelerating expansion. Ordinary matter, atoms, molecules, and radiation, also formed via the Higgs field, while energy, mostly electromagnetic radiation, fuels cosmic evolution. These pieces dance within a framework shaped by the Higgs, elusive quantum gravity, and the subtle interplay of dark matter and dark energy.

Could radiation, dark matter, and dark energy be different faces of a single, evolving force? Radiation transitioning to dark matter gradually shifting into dark energy, the universe might unravel, leaving isolated stars drifting in an endless void. Then, fluctuations in the Higgs field and quantum gravity could trigger contraction, setting the stage for another bounce. Rather than destruction, this might be a cosmic recycling, a continuous interplay of forces across time: Life, the Universe, and Everything.

Source: CDM Analogous to Superconductivity by Liang and Caldwell, May 2025, APS.org. Graphic: Cosmic Nebula by Margarita Balashova.

Web of Dark Shadows

Cold Dark Matter (CDM) comprises approximately 27% of the universe, yet its true nature remains unknown. Add that to the 68% of the universe made up of dark energy, an even greater mystery, and we arrive at an unsettling realization: 95% of the cosmos remains unexplained.

Socrates famously said, “The only thing I know is that I know nothing.” Over two millennia later, physicists might agree. But two researchers from Dartmouth propose a compelling possibility: perhaps early energetic radiation, such as photons, expanded and cooled into massive fermions, which later condensed into cold dark matter, the invisible force holding galaxies together. Over billions of years, this dark matter may be decomposing into dark energy, the force accelerating cosmic expansion.

Their theory centers on super-heavy fermions, particles a million times heavier than electrons, which behave in an unexpected way due to chiral symmetry breaking: where mirror-image particles become unequally distributed, favoring one over the other. Rather than invoking exotic physics, their model works within the framework of the Standard Model but takes it in an unexpected direction.

In the early universe, these massive fermions behaved like radiation, freely moving through space. However, as the cosmos expanded and cooled, they reached a critical threshold, undergoing a phase transition, much like how matter shifts between liquid, solid, and gas.

During this transformation, fermion-antifermion pairs condensed—similar to how electrons form Cooper pairs in superconductors, creating a stable, cold substance with minimal pressure and heat. This condensate became diffuse dark matter, shaping galaxies through its gravitational influence, acting as an invisible web counteracting their rotation and ensuring they don’t fly apart.

However, dark matter may not be as stable as once thought. The researchers propose that this condensate is slowly decaying, faster than standard cosmological models predict. This gradual decomposition feeds a long-lived energy source, possibly contributing to dark energy, the force responsible for the universe’s accelerated expansion.

A more radical interpretation, mine not the researchers, suggests that dark matter is not merely decaying, but evolving into dark energy, just as energetic fermion radiation once transitioned into dark matter. If this is true, dark matter and dark energy may be two phases of the same cosmic entity rather than separate forces.

If these hypothesis hold, we should be able to detect, as the researchers suggest, traces of this dark matter-to-dark energy transformation in the cosmic microwave background (CMB). Variations in density fluctuations and large-scale structures might reveal whether dark matter has been steadily shifting into dark energy, linking two of cosmology’s biggest unknowns into a single process.

Over billions of years, as dark matter transitions into dark energy, galaxies may slowly lose their gravitational cage and begin drifting apart. With dark energy accelerating the expansion, the universe may eventually reach a state where galaxies unravel completely, leaving only isolated stars in an endless void.

If dark matter started as a fine cosmic web, stabilizing galaxies, then over time, it may fade away completely, leaving behind only the accelerating force of dark energy. Instead of opposing forces locked in conflict, what if radiation, dark matter, and dark energy were simply different expressions of the same evolving entity?

A tetrahedron could symbolize this transformation:

  • Radiation (Energetic Era) – The expansive force that shaped the early universe.
  • Dark Matter (Structural Phase) – The stabilizing gravitational web forming galaxies.
  • Dark Energy (Expansion Phase) – The force accelerating cosmic evolution.
  • Time (Governing Force) – The missing element driving transitions between states.

Rather than the universe being torn apart by clashing forces, it might be engaged in a single, continuous transformation, a cosmic dance shaping the future of space.

Source: CDM Analogous to Superconductivity by Liang and Caldwell, May 2025, APS.org. Graphic: Galaxy and Spiderweb by Copilot.

Cosmic Halo

Galactic halos, consisting of a spherical envelope of dark matter along with sparsely scattered stars, globular clusters, and gas, typically surround most spiral galaxies. Current research is investigating the possibility that some halos may exist solely of dark matter. Discovering halos without stellar matter carries profound implications for our understanding of the universe’s structure, galaxy formation processes, and the conditions required for star formation. More importantly, such a discovery would provide a unique laboratory to study dark matter in isolation, free from interference of normal matter. However, new findings suggest that starless halos may be even rarer than previously thought. This scarcity makes detecting such halos particularly challenging, as they are unlikely to be associated with observable galaxies.

Ethan Nadler, of the University of California San Diego, has demonstrated that molecular hydrogen requires significantly less mass for star formation compared to atomic hydrogen. His research shows that molecular hydrogen can cool sufficiently for gravity to initiate star formation at lower mass thresholds. Specifically, while past studies indicated that dark matter halos need between 100 million to 1 billion solar masses of atomic hydrogen to begin star formation, Nadler has revealed that molecular hydrogen can achieve the same result with as little as 10 million solar masses—a reduction by a factor of 10 to 100. While dark matter halos can theoretically form with masses as low as 10⁻⁶ solar masses, depending on the nature of dark matter, those capable of influencing galaxy formation typically require at least 10⁶ solar masses to enable star formation, further highlighting the challenge of finding starless halos. Detecting these small, starless halos would require identifying subtle perturbations in gravitational fields, a difficult task that may yield little if such halos are as rare as current models suggest.

Source: …Galaxy Formation Threshold, Nadler, AAS, April 2025. Graphic: Dark Matter Halo Simulation by Cosmo0. Public Domain.

Fate of the Universe

Astronomers once observed exploding stars (supernovae) and found the universe expanding, driven by a mysterious force called dark energy. This led to the standard cosmological model of the late 1990s, Lambda-CDM, where “Lambda” represents dark energy, assumed constant, and “Cold Dark Matter” (CDM) explains unseen mass shaping cosmic structure. Evidence for CDM includes steady star rotation speeds in galaxies, cosmic microwave background fluctuations, galaxy clustering, and light bending by gravity. Though successful, Lambda-CDM has faced ongoing scrutiny almost from inception of the theory.

Enter the Dark Energy Spectroscopic Instrument (DESI) at Kitt Peak National Observatory in Arizona. With 5,000 robotic fiber-optic sensors, DESI captures light from galaxies and quasars, mapping the universe’s expansion history. A new study, analyzing three years of DESI data, 15 million objects, with plans for 50 million, combines it with cosmic microwave background radiation, supernovae, and weak gravitational lensing data. Fitting all this into Lambda-CDM with a constant dark energy revealed cracks in the model. But if dark energy weakens over time, a “dynamical dark energy“, the model aligns better.

By observing objects up to 11 billion years away, DESI peers deep into cosmic history. Researchers found hints that dark energy’s strength may have peaked around 7 billion years ago, then started weakening, challenging its fixed nature in Lambda-CDM. While not certain, this could rival the 1990s discovery of accelerated expansion, potentially demanding a new model.

The universe’s fate depends on dark energy versus matter. It’s been accelerating, but a weakening dark energy might slow it down, halt it, or, if gravity overtakes sufficiently, trigger a “Big Crunch.” New data from DESI, Europe’s Euclid, NASA’s Nancy Grace Roman, and Chile’s Vera Rubin Observatory could clarify this within five years, possibly nailing dark energy’s role.

Source: “Dark Energy Seems to Be Changing, Rattling Our View of Universe” by Rey and Lawler, Phys.org, March 2025. Graphic: DESI Collaboration Photo of Galaxies.

White Holes, Black Holes, and the Cosmic Cycle

White holes, theoretical counterparts to black holes, might be two sides of a cosmic coin. Black holes devour matter with relentless gravity; white holes expel it, hurling energy, particles, and possibly time into the universe. Both stem from Einstein’s general relativity, which predicts black holes, proven by solid evidence, while white holes remain elusive, perhaps lurking beyond our Earthly senses. 

To see their link, rethink black holes’ strangest feature and flaw: the singularity. General relativity paints it as a point where spacetime crushes so tight that physics breaks, a bug, not a feature. Exotic matter, with odd traits like negative energy, was once the fix. But the University of Barcelona’s Pablo Bueno and team ditched it, tweaking gravity with higher-curvature corrections to erase singularities. This needs extra dimensions beyond our four, turning black holes from traps into dynamic zones. 

The University of Sheffield adds a twist: the event horizon isn’t sharp. Quantum gravity blurs it into a fuzzy gateway where spacetime bends, not breaks. In 4D, black holes are sinkholes, matter vanishes. In higher dimensions, it slips through, heading elsewhere. Sheffield’s take ties this to dark energy, the universe’s expansion driver. Here, it’s the power plant: quantum fluctuations, fueled by dark energy, replace the singularity with a bounce, flipping spacetime to a white hole. 

Enter white holes, Janus-like transitions, Roman god of gates and duality. Black holes vacuum everything; white holes, linked via higher dimensions, spit it out, maybe far off. Picture Sagittarius A*, the Milky Way’s core black hole, channeling matter 25,000 light-years to the Orion Nebula’s arm. Unseen, white holes might hide in dimensions we can’t touch. 

This hints at a cosmic cycle, like Earth’s water cycle: evaporate, rain, repeat. Black holes swallow, dark energy and quantum gravity bounce it through higher dimensions, and white holes release it back. Barcelona and Sheffield suggest no endpoints, just a recycling of cosmic raw materials across realms we’re barely capable of understanding.

Source: Black Hole Singularity, Gielen and Menendez-Pidal, University of Sheffield, 2025. Regular Black Holes…by Bueno, P. et al, Physics Letter B, February 2025. Graphic: Black Hole Rendering.

Gravity and Vanilla Black Holes

Einstein’s theory of general relativity, which includes gravity, predicts that black holes have a tricky feature: a singularity. This is a point where space and time are squeezed so tightly that the laws of physics break down—think of it as a cosmic “error message.” To fix this, scientists often turn to exotic matter—hypothetical substances with bizarre properties like negative energy—to smooth things out. However, a team from the University of Barcelona, led by Pablo Bueno, found an alternative. They didn’t need exotic matter at all. Instead, they tweaked Einstein’s gravity by adding an infinite series of extra “rules” (higher-curvature corrections) to the math.

Their solution works in spacetimes with more than four dimensions—beyond our usual height, width, depth, and time. In these higher-dimensional worlds, black holes can exist without singularities. This “smooths out” black holes, making them less mysterious and more like regular objects in spacetime—no weird stuff required.

The presence of extra dimensions doesn’t just fix singularities—it can also change how black holes behave. In higher-dimensional spacetimes, black holes might have different event horizon shapes (the boundary beyond which nothing escapes) or other structural quirks. The Barcelona team’s work shows that these altered properties emerge naturally from gravity in more than four dimensions, offering a fresh perspective on these cosmic giants.

Thinking outside the box, is it possible that these extra dimensions link black holes to “a reality outside regular spacetime,” like wormholes (tunnels through spacetime), braneworlds (parallel universes on higher-dimensional “membranes”), or even gateways to white holes (theoretical opposites of black holes that spit stuff out)? Theories like string theory and braneworld scenarios suggest that extra dimensions might allow such connections. For example, a wormhole could theoretically bridge two distant points in our universe—or even lead to a completely different universe.

While the math of higher dimensions opens the door to these possibilities, it’s all conjecture. The Barcelona team’s work is a major step forward in understanding black holes in higher dimensions, but it doesn’t directly prove connections to other realities.

Source: Grok 3. Regular Black Holes… by Bueno, P. et al., Physics Letter B, February 2025. Graphic: Black Hole Rendering, iStock licensed.