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Measuring Energy at the Zeptojoule Level

A dive into the world of zeptojoule calorimetry and its significance.

András Gunyhó, Kassius Kohvakka, Qi-Ming Chen, Jean-Philippe Girard, Roope Kokkoniemi, Wei Liu, Mikko Möttönen

― 8 min read


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Table of Contents

In the vast universe of measuring energy, where every tiny amount counts, there’s a fascinating field called zeptojoule calorimetry. Now, zeptojoule might sound like something from a sci-fi movie, but it's actually a way of measuring energy at an unbelievably small scale—specifically, one-septillionth of a joule. To put that into perspective, that’s like measuring a single crumb of sugar in a huge bowl of sugar!

Why Do We Measure Energy?

What’s the big deal with measuring energy, you ask? Well, energy measurement is essential in many scientific fields. Imagine trying to understand the early universe, or figuring out how particles decay, or even making the gadgets we love to use every day, like smartphones and computers. Scientists need precise measurements to build accurate models. It’s like trying to assemble IKEA furniture without proper measurements—you might end up with a bizarre-looking chair instead of a bookshelf!

How Do Calorimeters Work?

Calorimeters are like the superheroes of energy measurement. They work by absorbing incoming energy (a fancy way of saying they catch it) and then turning that energy into heat. This heat creates a slight change in temperature, which can be detected and measured using a thermometer. It’s akin to how your phone gets warm when you’re using it for too long—even tiny amounts of energy can add up!

Some of the most sensitive calorimeters out there include bolometers and calorimeters. They have become the go-to devices for detecting energy because they can catch even the smallest amounts. Think of it like trying to hear a whisper in a noisy room—these devices are built to listen for even the faintest sounds of energy.

The Super Sensitive Calorimeters

Now, we’re not just talking about your average calorimeter here. The latest models, like transition edge sensors and magnetic microcalorimeters, can achieve an energy resolution as tiny as 17.6 zeptojoules. These devices are so sensitive that they could almost detect a butterfly flapping its wings from across the room!

Recently, even more advanced versions have emerged, using materials like graphene and Superconductors. Imagine two super cool materials having a dance party, and together they create a stellar energy detector. These new sensors predicted Energy Resolutions as low as 0.75 zeptojoules. The excitement in the lab was palpable—scientists were practically high-fiving each other!

The Challenges in Measuring Energy

Despite all the advancements, there’s a catch. Researchers have only managed to predict these tiny measurements mathematically. In real life, no one had demonstrated calorimetry achieving single zeptojoule energy resolution. It’s a bit like having the world’s best recipe for chocolate chip cookies but never actually baking them. Close, but no cookies!

Let’s Get Technical

In a recent endeavor, scientists decided to put their theories to the test. They used a metallic SNS (superconductor-normal-superconductor) sensor to measure the energy from 1-microsecond-long 8.4-GHz microwave pulses with impressive energy resolution below 1 zeptojoule. That’s like measuring a thunderstorm using a feather’s weight!

This energy resolution corresponds to roughly 170 Photons at that microwave frequency. You could almost imagine the photons high-fiving each other as they pass through the sensor. This significant achievement opened up exciting possibilities for real-time detection of single photons—those little light particles which are crucial in the technology of the future!

Why Should We Care?

But why should we care about detecting single photons? Well, this technology could lead to more accurate measurements in quantum computing, which is demanding for a lot of industries, including cryptography and telecommunications. If you’ve ever been frustrated by a slow internet connection, we could be on the verge of super-fast data transfer thanks to these advancements!

Moreover, the same technology has implications for fundamental physics, including the search for mysterious particles like axions—a particle that scientists suspect could play a role in explaining dark matter. The quest for knowledge never ends, and energy measurement plays a crucial role in this ongoing adventure.

The Race to Detection

Detecting weak electromagnetic signals has become a hot topic in various scientific fields. It’s like trying to catch a minnow in a river while standing on the shore—challenging but rewarding! Over the years, several ultra-sensitive radiation sensors have been developed, particularly those that operate at cryogenic temperatures (very, very cold!).

These sensors can detect individual microwave photons, but let’s be real: they usually can’t tell you how much energy those photons have. It’s like having the best camera but no clue about what the picture actually looks like. Researchers realized that in order to achieve energy resolution over a broad frequency band, they needed to find better techniques.

Breaking Down Cooper Pairs

One of the keys to energy resolution lies in sensors that can detect when incoming photons break Cooper pairs in superconductors. You could say that when photons arrive, it’s like they’re playing a game of tag, and when they touch a Cooper pair, chaos ensues! This is the basic principle for kinetic inductance detectors (KIDs), superconducting nanowire single-photon detectors, and quantum capacitance detectors (QCDs).

These sensors have seen success, with KIDs detecting individual photons and QCDs peeking at energies lower than a zeptojoule. However, it’s been a tough nut to crack—thermal detectors come with their limitations, primarily thermal fluctuations, while the fancy detectors don’t have energy resolution. It’s like trying to choose between two people for a date, but neither is a perfect match!

A New Player Enters the Game

In recent projects, researchers used metallic SNS sensors to break through the barrier of single-zeptojoule energy resolution. They first checked the noise equivalent power—in simple terms, how much noise the sensor makes—and then used that information to measure individual traces of the detector signal as they sent short microwave pulses into the sensor.

To make things even better, a matched filter was applied to the traces. It’s like putting on a pair of special glasses that help you see what was once blurry. This improved the signal-to-noise ratio, which is key for getting accurate readings. The outcome? An energy resolution finer than expected, putting these researchers ahead in the race for better energy detection methods.

How Does It All Work?

So how does this snazzy sensor work? Let’s break it down. The SNS radiation sensor consists of a microwave absorber and a thermometer. The absorber is like a sponge soaking up energy, while the thermometer senses the heat generated. The energy excites quasiparticles, effectively heating the absorber and shifting the thermometer’s readings.

This temperature change creates a shift in the resonance frequency—all fancy talk for saying that something moves when you apply energy. Researchers can then track that movement, which is how they can measure the energy input! The device is cooled down to chilly temperatures to maximize its sensitivity, and voilà—energy measured!

The Results Are In!

As scientists worked on this project, they managed to measure the time-domain signal in real life, rather than just predict it. They applied short microwave pulses of energy and recorded the traces. After applying a matched filter, they found the results were significantly clearer, leading to a better interpretation of the energy level.

In the end, they constructed cumulative distribution functions to analyze the calorimetric signals based on their findings. They discovered that the noise in the signal followed a normal distribution. Who knew that tiny energies could be so predictable?

Getting to the Bottom of It

The researchers estimated the resolution using mean values, standard deviations, and a smattering of statistics to see how well the calorimeter was performing. It turns out that with the right pulse energy, they could accurately measure energy with a resolution finer than some of the best detected before. This means that the device could potentially resolve single microwave photons—you know, the little guys that hold the key to so many questions in quantum physics!

Future Possibilities

With these advanced measuring capabilities, the sky’s not the limit. Scientists can now venture into realms previously thought unreachable. Imagine a world where we could measure energy at a single photon level in real time. The implications for quantum technology, astrophysics, and even our daily lives could be monumental.

Furthermore, researchers are keen to pursue enhancing energy measurement by exploring new materials and setups. Innovations like using graphene could lead to even further precision. It’s like upgrading from a regular bicycle to a rocket-powered one!

Conclusion: What’s Next?

In conclusion, zeptojoule calorimetry is almost like a roller coaster of excitement in the world of energy measurement. From tiny zeptojoules to the big questions of the universe, the journey of understanding energy continues. This breakthrough in sensitivity could lead to a plethora of applications, paving the way for advancements that could change the way we understand physics forever.

So, the next time you find yourself sipping tea while pondering the mysteries of the universe, remember that scientists are out there measuring energy at levels so small they’d make a flea look like a giant! Each small step in calorimetry gets us closer to unlocking the many secrets of life, the universe, and everything in between. Keep an eye on this field—it’s bound to get a whole lot more exciting!

Original Source

Title: Zeptojoule Calorimetry

Abstract: The measurement of energy is a fundamental tool used, for example, in exploring the early universe, characterizing particle decay processes, as well as in quantum technology and computing. Some of the most sensitive energy detectors are thermal, i.e., bolometers and calorimeters, which operate by absorbing incoming energy, converting it into heat, and reading out the resulting temperature change electrically using a thermometer. Extremely sensitive calorimeters, including transition edge sensors, magnetic microcalorimeters and devices based on 2D conductors such as graphene, have been shown to reach impressive energy resolutions of 17.6 zJ. Very recently superconductor--normal-conductor--superconductor (SNS) radiation sensors with metallic and graphene absorbers have resulted in predictions of full-width-at-half-maximum (FWHM) energy resolutions of 0.75 zJ and 0.05 zJ = 71 GHz$\times h$, respectively, where $h$ is the Planck constant. However, since these estimates are only mathematically extracted from steady-state noise and responsivity measurements, no calorimetry reaching single-zeptojoule energy resolution or beyond has been demonstrated. Here, we use a metallic SNS sensor to measure the energy of 1-$\mu$s-long 8.4-GHz microwave pulses with a FWHM energy resolution finer than (0.95 $\pm$ 0.02) zJ = (5.9 $\pm$ 0.12) meV, corresponding to 170 photons at 8.4 GHz. The techniques of this work, combined with graphene-based sensors, provide a promising path to real-time calorimetric detection of single photons in the 10 GHz range. Such a device has potential in operating as an accurate measurement device of quantum states such as those of superconducting qubits, or used in fundamental physics explorations including quantum thermodynamics, and the search for axions.

Authors: András Gunyhó, Kassius Kohvakka, Qi-Ming Chen, Jean-Philippe Girard, Roope Kokkoniemi, Wei Liu, Mikko Möttönen

Last Update: 2024-12-18 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2412.14079

Source PDF: https://arxiv.org/pdf/2412.14079

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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