Cosmology is the scientific study of the large-scale properties of the universe as a whole. It aims to understand the origin, evolution, structure, and eventual fate of the universe. By examining cosmic phenomena such as the Big Bang, cosmic microwave background radiation, dark matter, and dark energy, cosmologists develop theories and models that explain how … Read more
The quest for a Theory of Everything (TOE) is one of the most ambitious scientific endeavors, aiming to unify all fundamental forces and particles in a single, all-encompassing theoretical framework. This grand vision seeks to bridge the gap between the two main pillars of modern physics: General Relativity, which describes the macroscopic world of gravity … Read more
Researchers at the Research Center for the Early Universe (RESCEU) and the Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU, WPI) at the University of Tokyo have recently leveraged quantum field theory—traditionally applied to minute, subatomic phenomena—to explore the early universe. Their findings suggest that miniature black holes, specifically primordial black … Read more
The search for gravitational lenses is a fascinating endeavor in astronomy and cosmology that has revolutionized our understanding of the universe’s structure, composition, and evolution. Gravitational lenses are cosmic phenomena predicted by Einstein’s general theory of relativity, where the gravitational field of massive objects, such as galaxies or galaxy clusters, bends and distorts the paths … Read more
The future of space exploration holds tremendous promise and excitement, with ambitious plans, innovative technologies, and international collaborations poised to expand humanity’s reach into the cosmos. From returning humans to the Moon and exploring Mars to venturing deeper into the solar system and beyond, the next era of space exploration is set to unlock new … Read more
The origin and evolution of the universe have fascinated humanity for millennia. Modern scientific theories, such as the Big Bang theory, provide a framework for understanding these cosmic processes. The universe began as an unimaginably dense and hot singularity around 13.8 billion years ago, expanding rapidly and cooling over time. Through cosmic inflation, galaxies, stars, … Read more
Quasars, short for “quasi-stellar radio sources,” are among the most enigmatic and fascinating objects in the cosmos. They are incredibly bright and energetic, emitting radiation across the entire electromagnetic spectrum, from radio waves to X-rays and gamma rays. Quasars are powered by the accretion of material onto supermassive black holes at the centers of galaxies, … Read more
The dance of galaxies in the cosmic web is a mesmerizing spectacle of cosmic structure and evolution, revealing the intricate interplay of gravity, dark matter, and cosmic forces shaping the large-scale distribution of galaxies in the universe. The cosmic web is a vast network of filaments, voids, and clusters that connect galaxies across cosmic distances, … Read more
Gravitational waves are ripples in the fabric of spacetime caused by the acceleration of massive objects, such as merging black holes or neutron stars. Predicted by Albert Einstein’s theory of general relativity in 1915, these waves were detected for the first time in 2015, marking a revolutionary breakthrough in astrophysics and opening a new window … Read more
Dark matter is one of the most mysterious and elusive substances in the universe. Despite making up approximately 27% of the total mass-energy content of the cosmos, its nature remains largely unknown. Scientists have been working tirelessly for decades to unravel the secrets of dark matter, aiming to understand its properties, distribution, and role in … Read more
A UCL-led research team has used artificial intelligence (AI) techniques to infer the influence and properties of dark energy more precisely from a map of dark and visible matter in the universe covering the last 7 billion years. The study, submitted to the Monthly Notices of the Royal Astronomical Society and available on the arXiv preprint server, was carried … Read more
The rate at which the universe is expanding, known as the Hubble constant, is one of the fundamental parameters for understanding the evolution and ultimate fate of the cosmos. However, a persistent difference, called the Hubble Tension, is seen between the value of the constant measured with a wide range of independent distance indicators and … Read more
A team of physicists has developed a method to detect gravity waves with such low frequencies that they could unlock the secrets behind the early phases of mergers between supermassive black holes, the heaviest objects in the universe. The method can detect gravitational waves that oscillate just once every thousand years, 100 times slower than … Read more
We now have a standard model of cosmology, the current version of the Big Bang theory. Although it has proved very successful, its consequences are staggering. We know only 5% of the content of the universe, which is normal matter. The remaining 95% is made up of two exotic entities that have never been produced … Read more
Measuring the age of the universe, a question that has captivated astronomers and cosmologists for centuries, involves probing the depths of space and time to unravel the mysteries of cosmic evolution. Through a combination of theoretical models, observational data, and cutting-edge technologies, scientists have pieced together a remarkably detailed picture of the universe’s origins, composition, … Read more
Redshift, a fundamental concept in astronomy and cosmology, serves as a cornerstone for understanding the universe’s vastness, expansion, and evolution. It represents a phenomenon where the light emitted by celestial objects, such as galaxies, stars, and quasars, is shifted towards longer wavelengths as they move away from an observer. This phenomenon, discovered over a century … Read more
Cosmic inflation is a theoretical framework in cosmology that describes a rapid and exponential expansion of the early universe during the first few moments (10^-36 to 10^-32 seconds) after the Big Bang. Proposed in the late 1970s by physicist Alan Guth and independently by Andrei Linde, cosmic inflation provides a solution to several long-standing problems … Read more
Galaxies and nebulae are two captivating astronomical phenomena, each with distinct characteristics and roles in the vast tapestry of the universe. Understanding the differences between galaxies and nebulae is crucial in unraveling the complexities of cosmic structures, their formations, and their contributions to the cosmic landscape. A galaxy is an immense system of stars, stellar … Read more
The Hubble constant, denoted as H₀, is a fundamental parameter in cosmology that quantifies the rate at which the universe is expanding. Named after the American astronomer Edwin Hubble, who played a crucial role in the discovery of the expansion of the universe, this constant has been central to our understanding of cosmic evolution. Edwin … Read more
Gravitational waves are ripples in the fabric of spacetime caused by the acceleration of massive objects, such as merging black holes or neutron stars. First predicted by Albert Einstein in 1916 as part of his theory of general relativity, gravitational waves remained elusive for decades. It wasn’t until the 21st century that scientists successfully detected … Read more