Julian Muñoz has a ‘ruler’ that could size up the early universe


Julian Muñoz has provide you with a ruler to measure the early universe.

A theoretical physicist, Muñoz research the distant, dim interval within the universe’s historical past often known as cosmic daybreak. That’s when stars first started flickering on, a couple of hundred million years after the Huge Bang, infusing the universe with preliminary glimmers of starlight and forming the primary galaxies.

Earlier than the primary stars, the universe was chilly and darkish — as Muñoz describes it, “boring.” Then, starlight started to reshape the universe. “It’s a very dramatic epoch,” says Muñoz, of the College of Texas at Austin.

That epoch can be poorly understood. Cosmic daybreak is so unexplored that Muñoz compares it to an uncharted space on early maps of Earth. There, Muñoz says, “there might be dragons.” By learning this period, he hopes to disclose the conduct of 1 dragon of the cosmos, darkish matter, the inscrutable substance whose mass binds galaxies.

However to grasp the cosmos, scientists have to have the ability to measure it. Trying far into area means wanting deep into the previous. The difficulty is our 2-D view of the sky doesn’t readily reveal how distant issues are. “After we have a look at the night time sky, we’ve bought no depth notion,” says cosmologist Adrian Liu of McGill College in Montreal.

Scientists have devised quite a lot of strategies to get a deal with on distances, together with customary candles and customary rulers — objects of identified brightness or size. If you understand how shiny an object is (in contrast with how shiny it seems) or you understand how lengthy a selected characteristic is on the sky (in contrast with its obvious size), you may inform how distant it’s. A ruler appears to be like smaller from 20 meters away than from 10 meters away, and a 20-watt lightbulb appears to be like dimmer the farther away it’s. The identical applies over cosmic distances.

Scientists use sure sorts of exploding stars, for instance, to estimate distances, as a result of the blasts put out a predictable gentle present (SN: 5/8/12). Commonplace rulers or customary candles can be utilized to hint out how distant different objects of curiosity are and reveal how quickly the universe has expanded over its historical past.

However not one of the identified customary objects attain again to the cosmic daybreak period. That’s the place Muñoz’s ruler is available in. “This capacity to achieve that far again,” Liu says, “that’s the actually useful factor.”

Sizing up cosmic daybreak

Nobody has ever seen a conclusive signature of cosmic daybreak — the very first galaxies are too distant to watch instantly. However there’s one other approach to spot cosmic daybreak’s results, one which’s been a long-sought goal for astronomers. As the primary stars shaped, their gentle heated the encompassing hydrogen gasoline, inflicting it to soak up gentle with a wavelength of 21 centimeters, a quantity that outcomes from the separation between power ranges in hydrogen atoms. Observing that 21-centimeter absorption sign is the intention of the Hydrogen Epoch of Reionization Array, or HERA, collaboration, an effort that Muñoz and Liu each work on, utilizing a radio telescope in South Africa.

If it may be detected, this absorption sign ought to have delicate, ring-shaped patterns imprinted in it, Muñoz reported in 2019 in Bodily Evaluation Letters.

A computer simulation outputting the cosmic dawn era, shown mostly as a blend of dark blue and red splotches, with a double-sided arrow centered in the upper third
Secrets and techniques of the universe’s cosmic daybreak period are revealed in patterns of the absorption of sunshine with a 21-centimeter wavelength, proven in a pc simulation. Areas with extra absorption (purple) correspond to denser pockets of stars, in contrast with sparsely populated areas with much less absorption (blue). Sparse areas are typically separated by distances of about half a billion light-years (arrow signifies one instance); the identical goes for dense areas.J.B. Muñoz

These patterns, the idea of his ruler, consequence from the differing conduct of darkish matter and regular matter throughout an excellent ancient times, lower than 400,000 years after the Huge Bang. Sound waves careening via the plasma at the moment would have pushed regular matter to excessive speeds whereas leaving darkish matter at a standstill.

This mismatch in velocities affected the place galaxies shaped through the later cosmic daybreak period. To create a galaxy, darkish matter should gravitationally reel in regular matter. However the place the velocities differed, the conventional matter zipped proper on by. The early universe was left with sparsely populated areas of the sky, organized in ring-shaped patterns with a predictable distance scale. The rings, that are too delicate to pick by eye from the info however present up in statistical analyses, have radii of half a billion light-years – that’s one lengthy measuring stick.

The brand new customary ruler might reveal how briskly the universe was increasing again then. That info can inform scientists what that youthful universe was manufactured from, revealing the quantity of darkish matter, regular matter and darkish power, one other hidden piece of the cosmic puzzle.

A brand new growth measurement might additionally add gasoline to one of many fiercest debates in cosmology. At the moment, completely different measurements of the universe’s growth charge conflict with each other, leaving scientists pondering whether or not there are flaws in our understanding of the cosmos.

Looking for to grasp the unknown, together with these shadowy cosmic realms, is “an integral part of human nature — like artwork and poetry,” Muñoz says. “You may stay with out it, however I actually hope you don’t must.”

Trying into darkish corners

Muñoz’s curiosity in darkish matter drew him to the cosmic daybreak. The primary galaxies grew off a scaffold of darkish matter. So details about how and when these galaxies shaped can reveal darkish matter’s properties. In a report printed in 2018 in Nature, for instance, Muñoz and colleagues steered that, if a number of the universe’s darkish matter had a tiny electrical cost, a millionth of an electron’s, that might alter the anticipated cosmic daybreak sign.

He has additionally developed essential computational instruments, like a brand new method that permits for lightning-fast simulations of the cosmic daybreak, reported in Might in Month-to-month Notices of the Royal Astronomical Society. The time it takes to carry out these simulations has beforehand restricted what scientists can examine.

“He’s bought a watch for fascinating concepts,” says theoretical physicist Marc Kamionkowski of Johns Hopkins College, Muñoz’s Ph.D. adviser. However the cosmic ruler, “that’s most likely probably the most singular concept that he’s had.”

Turning into a physicist, in itself, was uncharted territory for Muñoz. As a toddler, he preferred science. He remembers being amazed by fossilized shark enamel that had been hundreds of thousands of years previous — maybe his first expertise grappling with such grand timescales.

However Muñoz didn’t have a scientific position mannequin; his mother and father didn’t end highschool. He targeted his consideration on video video games and coding till a highschool physics instructor inspired his scientific streak. He turned to physics, he says, the place “it was potential to channel all this nerdy power for information.” That’s what drives Muñoz to discover the questions that swirl round darkish corners of the cosmos. “I do it as a result of I feel the solutions enrich the human expertise.”


Julian Muñoz is one in all this 12 months’s SN 10: Scientists to Watch, our listing of 10 early and mid-career scientists who’re making extraordinary contributions to their discipline. We’ll be rolling out the complete listing all through 2023.

Wish to nominate somebody for the SN 10? Ship their title, affiliation and some sentences about them and their work to sn10@sciencenews.org.