Space is getting bigger.
It is growing very fast. A hidden force helps it grow. This force is in empty space. It helps the whole universe move. Do you like looking at the stars?
Space is growing very fast.
A hidden force helps it grow. This force is in empty space. A man named Albert Einstein first thought of it. He wanted space to stay still. But he found out that space moves.
Later, scientists saw that space grows even faster. This happens because of a special energy. It is like a push that fills the sky. Most of the universe is made of this energy.
It is a big mystery for us to solve.
The universe is growing. It is even growing faster every day. This happens because of a special force. Scientists call this the cosmological constant.
Albert Einstein first thought of this idea in 1917. He wanted the universe to stay still. He thought gravity would pull everything together. He added a new part to his math to stop this. He wanted to keep the universe steady. But he was wrong. Edwin Hubble found that the universe is actually growing. Einstein called his mistake his "biggest blunder."
Many years later, scientists found something new. In 1998, teams studied distant stars. They found the universe is speeding up. This speed-up is caused by dark energy. The cosmological constant helps explain this dark energy.
Dark energy is very big. It makes up about 68% of the universe.
This energy lives in empty space. It is a great mystery. Scientists are still trying to learn why it works this way.
The universe is much more than just empty space. It is filled with a mysterious force that helps explain how everything moves. Scientists call this force the cosmological constant. This idea is a key part of the standard model of cosmology, known as the ΛCDM model. It is closely linked to a concept called dark energy. Dark energy acts like a repulsive force that pushes things apart. This force fights against the pull of gravity.
To understand how it works, think about how gravity pulls things together. Without any other force, gravity would make the universe shrink. The cosmological constant provides a way to describe the energy density of space. This is also called vacuum energy. In quantum mechanics, even empty space is not truly empty. It is made of quantum fields that have tiny fluctuations. These fluctuations create a small amount of energy everywhere in space. This energy can drive the expansion of the universe.
Albert Einstein first introduced this idea in 1917. He added it to his math to keep the universe static. At that time, most people thought the universe did not change. Einstein wanted to stop gravity from making the universe collapse. However, Edwin Hubble discovered in 1929 that the universe is actually expanding. Einstein later called his attempt to keep the universe still his "biggest blunder." For many years, most scientists thought the constant was zero.
In 1998, everything changed with a new discovery. Two different teams of scientists studied distant stars called type Ia supernovae. Saul Perlmutter, Brian Schmidt, and Adam Riess led these important studies. They expected to see the expansion of the universe slowing down. Instead, they found that the expansion is actually speeding up. This means the universe is undergoing accelerated expansion. Because of this work, these three scientists won the Nobel Prize in 2011.
Today, we know that dark energy is a huge part of our world. It makes up about 68% of the mass-energy density of the universe. This is a much larger amount than the matter we can see. Scientists use the cosmological constant to explain this huge amount of energy. However, there is still a massive mystery called the cosmological constant problem. The math for vacuum energy predicts a value much larger than what we see. This gap is one of the greatest mysteries in all of science.
The cosmological constant, often written as the Greek letter lambda ($\Lambda$), is a mathematical term used to describe the energy density of space. In modern physics, it is the simplest way to explain dark energy. Dark energy is a mysterious force that acts as a repulsive pressure. This pressure pushes against the inward pull of gravity. The cosmological constant is a vital part of the $\Lambda$CDM model. This is the standard model used by scientists to describe how our universe works.
To understand how it works, we must look at the energy within empty space. According to quantum field theory, empty space is not truly empty. It is made of many different quantum fields. These fields experience tiny fluctuations in their lowest energy state, known as the vacuum state. These fluctuations create what scientists call zero-point energy. This energy exists everywhere in space. When this vacuum energy is positive, it creates a negative pressure. This negative pressure drives the accelerated expansion of the universe.
There are different ways to look at this energy in the universe. One way is through the density parameter, denoted as $\Omega_{\Lambda}$. This represents the ratio of dark energy density to the critical density of the universe. The critical density is the specific amount of energy needed to stop the universe from expanding forever. Another way is through the equation of state, denoted as $w$. This ratio compares the pressure of dark energy to its energy density. For a cosmological constant, this value is exactly -1. This specific value is consistent with observations from the Planck Collaboration in 2018.
Albert Einstein first introduced the cosmological constant in 1917. He added it to his field equations for general relativity. At that time, scientists believed the universe was static and eternal. However, Einstein's original equations suggested that gravity would cause a non-expanding universe to contract. He added the constant to counterbalance gravity and achieve a stable, static universe. He was not happy with this addition. He later called it an "ugly thing" and felt a "bad conscience" about it.
Einstein's static model did not last long. In 1922, the mathematician Alexander Friedmann showed that his equations allowed for a dynamic universe. Then, in 1929, Edwin Hubble provided astronomical evidence that the universe was actually expanding. This discovery meant the cosmological constant was not needed to keep the universe static. Einstein reportedly called his attempt to create a static universe his "biggest blunder." For many decades, most physicists assumed the value of the cosmological constant was zero.
In 1998, a major discovery changed everything. Two separate teams, the Supernova Cosmology Project and the High-Z Supernova Search Team, studied type Ia supernovae. These are distant exploding stars used to measure cosmic distances. The scientists expected to see the expansion of the universe slowing down due to gravity. Instead, they found that the expansion is actually accelerating. This meant the universe must have a positive cosmological constant. For this discovery, Saul Perlmutter, Brian Schmidt, and Adam Riess received the Nobel Prize in Physics in 2011.
This discovery has huge implications for the composition of our universe. Based on the cosmological principle, dark energy accounts for about 68% of the mass-energy density of the universe. This is a massive proportion compared to all other matter.
However, this leads to the "cosmological constant problem." This is one of the greatest mysteries in science. Quantum field theory predicts a vacuum energy that is much larger than what we actually observe. The predicted value exceeds the observed value by about 120 orders of magnitude. This massive gap is often called the worst theoretical prediction in the history of physics.
The study of the cosmological constant connects many different fields of science. It links the very large scale of general relativity with the very small scale of quantum mechanics. Many physicists believe that understanding the vacuum holds the key to a full understanding of nature. By studying how space expands, scientists hope to bridge the gap between these two major theories.
Where will your curiosity go next?
🖼️ Images & Media (3)
More to explore
✨ What else?
Related topics you might enjoy
🔬 Go deeper
More advanced topics to explore
🪜 Step back
Simpler topics to build understanding
What is Nepedia?
A free, ad-free encyclopedia for children. Every article is written at five reading levels, so the same page works for a five-year-old and a fifteen-year-old — use the level switcher above to see this one change. No account needed to read.