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Background Radiation and Quantum Computing

How background radiation impacts the future of quantum technology.

Joseph Fowler, Ian Fogarty Florang, Nathan Nakamura, Daniel Swetz, Paul Szypryt, Joel Ullom

― 6 min read


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We live in a world filled with hidden dangers, like Background Radiation. Radiation is not just a sci-fi plot device; it’s a real and ever-present part of our lives. In the context of quantum computing, this radiation can mess with Qubits-those funky little bits of data that can do more than just represent a 0 or a 1. They can be both at the same time! But before we get too carried away with the magic of quantum computing, let’s take a closer look at what background radiation really is and why we need to care about it.

What Is Background Radiation?

Background radiation comes from two main sources: natural and cosmic. The natural kind is all around us, lurking in the walls of our buildings, in the ground beneath our feet, and even in the food we eat. It’s like that friend who always shows up uninvited to parties-sometimes it’s a little annoying, but it’s hard to get rid of.

Cosmic Radiation, on the other hand, comes from outer space. Think of it as the universe's way of saying hello. These rays are high-energy particles that are zipping through space and can rain down on our planet. So, while you might be worried about the weather, there’s also a shower of cosmic rays happening all the time above our heads.

How Does Radiation Affect Qubits?

You might wonder how these sneaky rays affect qubits. Well, qubits are incredibly delicate and can be influenced by outside forces, including radiation. When background radiation hits a qubit, it can cause something called Decoherence. Basically, this means the qubit can lose its special magic state and revert to behaving more like a simple piece of data, losing its potential to perform complex calculations.

Imagine you're trying to balance two spoons on your nose while texting your friend. Everything's going well until a gust of wind (aka radiation) comes along and knocks one of those spoons off. Suddenly, it’s a lot harder for you to keep that balance! That’s what happens to qubits when radiation messes with them-they suddenly can’t do their job as well.

Types of Background Radiation

Natural Radiation

Now, let's break down background radiation a bit further. Natural radiation comes from various sources, including:

  • Building Materials: Yep, your house is giving off radiation! Materials, such as concrete, brick, and even some types of granite, can contain radioactive elements. Not exactly the cozy, warm feeling we want from our homes, right?

  • Soil and Rocks: The ground under our feet is like a geology buffet of radioactive elements. Some isotopes decay naturally, producing radiation.

  • Radon Gas: Radon is a sneaky gas formed from the decay of uranium, and it can seep into our homes. It's like that relative who visits and then never leaves.

Cosmic Radiation

Cosmic radiation adds another layer of complexity. This radiation is composed mainly of high-energy particles from outside our atmosphere, and it can vary depending on factors such as:

  • Altitude: The higher you go, the more cosmic rays you encounter. That’s why an airplane flight can expose you to more radiation than your average day at the beach.

  • Solar Activity: Think of the sun as a big, fiery ball that can sometimes sneeze, sending waves of particles towards Earth. During solar flares, those cosmic rays increase. So if you're planning a picnic on a sunny day, you might want to check the solar forecast!

The Simulation Game

Now, if all this sounds a little scary, don’t worry. Scientists have developed models to help us understand and predict how background radiation affects qubits and other sensitive instruments. They use high-tech tools like simulations to get a handle on the chaotic world of radiation.

Imagine you're a chef trying to bake the perfect cake. You need to consider all the ingredients and how they interact. Similarly, researchers simulate conditions to see how different materials and shielding can change the levels of background radiation impacting qubits.

Simulation Steps

  1. Setup: Researchers first design a model that represents a real-world scenario, like placing a qubit inside a laboratory setup.

  2. Shielding: Just like wearing sunscreen at the beach can protect your skin from harmful rays, researchers simulate the effects of various barriers or “shielding” materials. These shields can be made from concrete, aluminum, or a mix of both.

  3. Data Collection: After setting up the simulation, researchers can look at how much energy is deposited in the qubit. This is similar to measuring how many chocolate chips fit into your cookie recipe to achieve gooey perfection!

Key Rates of Radiation Effects

Researchers track a few important rates when measuring background radiation's effects:

  1. Event Rate: This refers to the number of times radiation hits the qubit and causes it to release energy. The more events, the more significant the effect on the qubit.

  2. Energy Deposition Rate: This captures how much energy is deposited into the qubit from these hits. More energy could lead to more significant issues with decoherence.

  3. Threshold Events: Certain energy levels, like one million electron volts (MeV), are important because they represent a shift in the kind of radiation interactions happening with the qubit.

Cosmic Rays vs. Terrestrial Gamma Rays

While both cosmic rays and terrestrial gamma rays cause trouble for qubits, they act differently.

  • Gamma Rays: These rays originate from radioactive elements in the ground. They can penetrate materials quite well. Think of them as the overachievers of the radiation world; they’re always eager to get involved!

  • Cosmic Rays: These high-energy particles can create a ruckus when they hit the atmosphere, resulting in a variety of secondary particles that hit the ground. They’re like a surprise party-exciting but also potentially disruptive!

Practical Implications

Researchers want to mitigate the effects of background radiation on quantum devices. Knowing the rates and impacts of radiation helps in creating more robust qubits less likely to lose their special properties.

Just like wearing a helmet while biking helps protect your noggin, implementing effective shielding can keep qubits functioning at peak performance. This way, we can advance quantum computing without worrying too much about those pesky background radiation effects.

The Bottom Line

In summary, background radiation is a real and constant part of our world, affecting everything from your morning cup of coffee to cutting-edge quantum computers. Scientists are working hard to model and predict these effects, and their findings could pave the way for better-performing qubits.

So next time you hear about the wonders of quantum computing, remember that even the most advanced technology has to deal with good old radiation. It’s a big universe out there, and we're all just trying to figure it out-one qubit at a time!

Original Source

Title: Computed models of natural radiation backgrounds in qubits and superconducting detectors

Abstract: Naturally occurring radiation backgrounds cause correlated decoherence events in superconducting qubits. These backgrounds include both gamma rays produced by terrestrial radioisotopes and cosmic rays. We use the particle-transport code Geant4 and the PARMA summary of the cosmic-ray spectrum to model both sources of natural radiation and to study their effects in the typical substrates used in superconducting electronics. We focus especially on three rates that summarize radiation's effect on substrates. We give analytic expressions for these rates, and how they depend upon parameters including laboratory elevation, substrate material, ceiling thickness, and wafer area and thickness. The modeled rates and the distribution of event energies are consistent with our earlier measurement of radiation backgrounds using a silicon thermal kinetic-inductance detector.

Authors: Joseph Fowler, Ian Fogarty Florang, Nathan Nakamura, Daniel Swetz, Paul Szypryt, Joel Ullom

Last Update: 2024-11-25 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2411.16974

Source PDF: https://arxiv.org/pdf/2411.16974

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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