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The Stability of Fundamental Constants Over Time

New findings suggest fundamental constants may remain unchanged throughout the universe's history.

Ze-Fan Wang, Lei Lei, Lei Feng, Yi-Zhong Fan

― 6 min read


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Have you ever wondered if the rules of our universe change over time? What if the things we take for granted, like the way light behaves or how gravity pulls us down, aren't as constant as we think? Scientists have been asking these very questions, especially when it comes to tiny numbers known as Fundamental Constants. These are the pillars of physics. They govern everything, from how atoms behave to how galaxies form.

Recently, a new telescope, the James Webb Space Telescope (JWST), has given us some amazing glimpses into the distant universe. With its fancy new tools, it's shedding light on these constants and whether they have been switching things up over time. For many, the thought of changing constants is as wild as imagining cats learning to play the piano, yet here we are!

What Are Fundamental Constants?

Let’s break it down a bit. Fundamental constants are numbers that appear in important equations in physics. They help us understand how the universe works. For example, there’s a constant related to electromagnetism, which affects how charged particles like electrons interact. There’s also the gravitational constant, which helps us understand how masses attract each other.

Now, most scientists assume these constants have stayed the same throughout the history of the universe. But what if they haven’t? Perhaps they’ve changed over billions of years, like fashion trends but less stylish.

No Ordinary Telescope

The JWST is not your average telescope. It’s like the superhero of space observation. Launched into space, it’s peering deep into the universe, looking at some of the oldest galaxies. With its powerful tools, it can analyze light in ways that previous telescopes like Hubble could only dream of.

With JWST’s help, scientists can study galaxies that formed just after the Big Bang! It’s like having a time machine, except instead of visiting your past, it’s all about observing the past of the universe.

Picking the Right Galaxies

To investigate our cosmic constants, researchers focused on a specific type of galaxy. These are called Emission Line Galaxies, which are essentially factories of light. They emit strong signals in certain parts of the spectrum, specifically in the infrared range. The researchers were like detectives on a mission, scouring the skies for these particular galaxies.

They specifically looked for two galaxies located quite far from us, at high redshifts, which means they are moving away quickly. This can happen because the universe is expanding, and faraway galaxies are generally older, giving us a glimpse into how things used to be.

Using Emission Lines as Clues

When researchers study these galaxies, they look at the light emitted from them. Imagine if a galaxy were a concert, and the light it sends out is like music. Different notes (or wavelengths) tell a story about what’s going on inside.

In this case, the clues came from two specific wavelengths of light emitted by oxygen, cleverly named [OIII]. These emissions are like shining flashlights that help scientists detect changes in cosmic constants. By analyzing these lights, they can gather information about the universe when it was very young.

The Evidence They Found

After gathering their data and examining these galaxies, the researchers found something interesting. The fine structure constant, which is a measure of the strength of electromagnetic forces, did not seem to change much. It remained consistent, like a dependable friend who never forgets your birthday.

This finding was exciting because it suggested that, at least in this case, our understanding of physical laws holds true across vast stretches of time. They looked at how this constant might have varied in the early universe and concluded that it has likely stayed stable since then.

Dark Energy and Its Mysterious Role

Now let’s throw another curveball into the mix: dark energy. This elusive force is believed to be driving the acceleration of the universe’s expansion. It’s like the universe’s version of that friend who always orders more appetizers when you’re not looking.

This dark energy might interact with electromagnetism, potentially affecting the fine structure constant. By looking at the relationship between dark energy and the constants of nature, scientists can further explore how they influence each other.

The researchers used their observations of the [OIII] emissions to set limits on how strong this interaction might be. They found that the strength of this coupling is likely very small, meaning dark energy and electromagnetism don’t play a wild tug-of-war over the universe’s behavior.

The Challenges of Collecting Data

Gathering data from distant galaxies isn’t as easy as ordering pizza. There are all sorts of challenges. For one, light can be absorbed by different materials out there in the cosmos. This can distort how we perceive what’s really happening in those far-off galaxies.

Also, the wavelengths of light that researchers are interested in can easily get skewed. Accurately measuring them requires precise tools and careful planning. The JWST is incredibly advanced, but even it has to deal with the quirks of cosmic light.

Looking Ahead

Researchers are still very excited about where this will lead. With the JWST’s continuous observations, they can now investigate other aspects of cosmic evolution. They may even refine how they measure these fundamental constants and improve their understanding of dark energy.

The universe is vast, and the mystery of how it works is still largely unsolved. But with each new piece of data, we get a little closer to forming a complete picture.

Conclusion

So, what have we learned? Fundamental constants appear to remain constant over time, at least according to the data gathered so far. The dark energy-electromagnetism interaction seems to be minimal.

Ultimately, the JWST is opening new doors, allowing scientists to ask bold new questions about the universe’s makeup. While the intricacies of fundamental constants may sound complicated, they form the very fabric of our reality. And thanks to the hard work of scientists and the powerful technology at their disposal, we’re unraveling this mystery one galaxy at a time.

In the end, the universe may not be changing its rules as much as we thought. But with so many stars and galaxies out there, who knows what else is waiting to be discovered?

Original Source

Title: JWST observations constrain the time evolution of fine structure constants and dark energy - electromagnetic coupling

Abstract: It was hypothesized in the literature that some physical parameters may be time-evolving and the astrophysical data can serve as a probe. Recently, James Webb Space Telescope (JWST) have released its early observations. In this work, we select the JWST spectroscopic observations of the high redshift ($z>7.1$) galaxies with strong [OIII] ($\lambda=4959$ \AA \,and $5007$ \AA \,in the rest frame) emission lines to constraint the evolution of the fine structure constant ($\alpha$). With the spectra from two galaxies at redshifts of $7.19$ and $8.47$, the deviation of $\alpha$ to its fiducial value is found to be as small as $0.44^{+8.4+1.7}_{-8.3-1.7} \times 10^{-4}$ and $-10.0^{+18+1.5}_{-18-1.5} \times 10^{-4}$, respectively (the first error is statistical and the latter is systematic). The combination of our results with the previous data reveals that $\frac{1}{\alpha} \frac{d \alpha}{dt} = 0.30^{+4.5}_{-4.5} \times 10^{-17}~{\rm yr^{-1}}$. Clearly, there is no evidence for a cosmic evolution of $\alpha$. The prospect of further constraining the time evolution of $\alpha$ is also discussed. The scalar field of dark energy is hypothesized to drive the acceleration of the universe's expansion through an interaction with the electromagnetic field. By integrating the observational data of the fine-structure constant variation, $\frac{\Delta\alpha}{\alpha}(z)$, we have established a stringent upper limit on the coupling strength between dark energy and electromagnetism. Our analysis yields $\zeta \leq 3.92 \times 10^{-7}$ at the 95\% confidence level, representing the most stringent bound to date.

Authors: Ze-Fan Wang, Lei Lei, Lei Feng, Yi-Zhong Fan

Last Update: 2024-11-13 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2411.08774

Source PDF: https://arxiv.org/pdf/2411.08774

Licence: https://creativecommons.org/licenses/by/4.0/

Changes: This summary was created with assistance from AI and may have inaccuracies. For accurate information, please refer to the original source documents linked here.

Thank you to arxiv for use of its open access interoperability.

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