Faster access than browser!Similarities between Lambda-CDM model and Universe
Lambda-CDM model and Universe have 41 things in common (in Unionpedia): Accelerating expansion of the universe, Age of the universe, Baryon, Baryon acoustic oscillations, Big Bang, Big Bang nucleosynthesis, Big Crunch, Cold dark matter, Cosmic Background Explorer, Cosmic microwave background, Cosmological constant, Cosmological principle, Dark energy, Dark matter, Dimensionless quantity, Einstein field equations, Expansion of the universe, Friedmann equations, Friedmann–Lemaître–Robertson–Walker metric, General relativity, Hot dark matter, Hubble's law, Illustris project, Inflation (cosmology), Isotropy, Monthly Notices of the Royal Astronomical Society, Neutrino, Parsec, Physical cosmology, Planck (spacecraft), ..., Quintessence (physics), Redshift, Reionization, Scale factor (cosmology), Shape of the universe, Spacetime, Standard Model, Theory of everything, Vacuum energy, Weak gravitational lensing, Wilkinson Microwave Anisotropy Probe. Expand index (11 more) »
Accelerating expansion of the universe
The accelerating expansion of the universe is the observation that the universe appears to be expanding at an increasing rate, so that the velocity at which a distant galaxy is receding from the observer is continuously increasing with time.
Accelerating expansion of the universe and Lambda-CDM model · Accelerating expansion of the universe and Universe ·
Age of the universe
In physical cosmology, the age of the universe is the time elapsed since the Big Bang.
Age of the universe and Lambda-CDM model · Age of the universe and Universe ·
Baryon
A baryon is a composite subatomic particle made up of three quarks (a triquark, as distinct from mesons, which are composed of one quark and one antiquark).
Baryon and Lambda-CDM model · Baryon and Universe ·
Baryon acoustic oscillations
In cosmology, baryon acoustic oscillations (BAO) are regular, periodic fluctuations in the density of the visible baryonic matter (normal matter) of the universe.
Baryon acoustic oscillations and Lambda-CDM model · Baryon acoustic oscillations and Universe ·
Big Bang
The Big Bang theory is the prevailing cosmological model for the universe from the earliest known periods through its subsequent large-scale evolution.
Big Bang and Lambda-CDM model · Big Bang and Universe ·
Big Bang nucleosynthesis
In physical cosmology, Big Bang nucleosynthesis (abbreviated BBN, also known as primordial nucleosynthesis, arch(a)eonucleosynthesis, archonucleosynthesis, protonucleosynthesis and pal(a)eonucleosynthesis) refers to the production of nuclei other than those of the lightest isotope of hydrogen (hydrogen-1, 1H, having a single proton as a nucleus) during the early phases of the Universe.
Big Bang nucleosynthesis and Lambda-CDM model · Big Bang nucleosynthesis and Universe ·
Big Crunch
The Big Crunch is one possible scenario for the ultimate fate of the universe, in which the metric expansion of space eventually reverses and the universe recollapses, ultimately causing the cosmic scale factor to reach zero or causing a reformation of the universe starting with another Big Bang.
Big Crunch and Lambda-CDM model · Big Crunch and Universe ·
Cold dark matter
In cosmology and physics, cold dark matter (CDM) is a hypothetical form of dark matter whose particles moved slowly compared to the speed of light (the cold in CDM) since the universe was approximately one year old (a time when the cosmic particle horizon contained the mass of one typical galaxy); and interact very weakly with ordinary matter and electromagnetic radiation (the dark in CDM).
Cold dark matter and Lambda-CDM model · Cold dark matter and Universe ·
Cosmic Background Explorer
The Cosmic Background Explorer (COBE), also referred to as Explorer 66, was a satellite dedicated to cosmology, which operated from 1989 to 1993.
Cosmic Background Explorer and Lambda-CDM model · Cosmic Background Explorer and Universe ·
Cosmic microwave background
The cosmic microwave background (CMB, CMBR) is electromagnetic radiation as a remnant from an early stage of the universe in Big Bang cosmology.
Cosmic microwave background and Lambda-CDM model · Cosmic microwave background and Universe ·
Cosmological constant
In cosmology, the cosmological constant (usually denoted by the Greek capital letter lambda: Λ) is the value of the energy density of the vacuum of space.
Cosmological constant and Lambda-CDM model · Cosmological constant and Universe ·
Cosmological principle
In modern physical cosmology, the cosmological principle is the notion that the spatial distribution of matter in the universe is homogeneous and isotropic when viewed on a large enough scale, since the forces are expected to act uniformly throughout the universe, and should, therefore, produce no observable irregularities in the large-scale structuring over the course of evolution of the matter field that was initially laid down by the Big Bang.
Cosmological principle and Lambda-CDM model · Cosmological principle and Universe ·
Dark energy
In physical cosmology and astronomy, dark energy is an unknown form of energy which is hypothesized to permeate all of space, tending to accelerate the expansion of the universe.
Dark energy and Lambda-CDM model · Dark energy and Universe ·
Dark matter
Dark matter is a theorized form of matter that is thought to account for approximately 80% of the matter in the universe, and about a quarter of its total energy density.
Dark matter and Lambda-CDM model · Dark matter and Universe ·
Dimensionless quantity
In dimensional analysis, a dimensionless quantity is a quantity to which no physical dimension is assigned.
Dimensionless quantity and Lambda-CDM model · Dimensionless quantity and Universe ·
Einstein field equations
The Einstein field equations (EFE; also known as Einstein's equations) comprise the set of 10 equations in Albert Einstein's general theory of relativity that describe the fundamental interaction of gravitation as a result of spacetime being curved by mass and energy.
Einstein field equations and Lambda-CDM model · Einstein field equations and Universe ·
Expansion of the universe
The expansion of the universe is the increase of the distance between two distant parts of the universe with time.
Expansion of the universe and Lambda-CDM model · Expansion of the universe and Universe ·
Friedmann equations
The Friedmann equations are a set of equations in physical cosmology that govern the expansion of space in homogeneous and isotropic models of the universe within the context of general relativity.
Friedmann equations and Lambda-CDM model · Friedmann equations and Universe ·
Friedmann–Lemaître–Robertson–Walker metric
The Friedmann–Lemaître–Robertson–Walker (FLRW) metric is an exact solution of Einstein's field equations of general relativity; it describes a homogeneous, isotropic, expanding or contracting universe that is path connected, but not necessarily simply connected.
Friedmann–Lemaître–Robertson–Walker metric and Lambda-CDM model · Friedmann–Lemaître–Robertson–Walker metric and Universe ·
General relativity
General relativity (GR, also known as the general theory of relativity or GTR) is the geometric theory of gravitation published by Albert Einstein in 1915 and the current description of gravitation in modern physics.
General relativity and Lambda-CDM model · General relativity and Universe ·
Hot dark matter
Hot dark matter (HDM) is a theoretical form of dark matter which consists of particles that travel with ultrarelativistic velocities.
Hot dark matter and Lambda-CDM model · Hot dark matter and Universe ·
Hubble's law
Hubble's law is the name for the observation in physical cosmology that.
Hubble's law and Lambda-CDM model · Hubble's law and Universe ·
Illustris project
The Illustris project is an ongoing series of astrophysical simulations run by an international collaboration of scientists.
Illustris project and Lambda-CDM model · Illustris project and Universe ·
Inflation (cosmology)
In physical cosmology, cosmic inflation, cosmological inflation, or just inflation, is a theory of exponential expansion of space in the early universe.
Inflation (cosmology) and Lambda-CDM model · Inflation (cosmology) and Universe ·
Isotropy
Isotropy is uniformity in all orientations; it is derived from the Greek isos (ἴσος, "equal") and tropos (τρόπος, "way").
Isotropy and Lambda-CDM model · Isotropy and Universe ·
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society (MNRAS) is a peer-reviewed scientific journal covering research in astronomy and astrophysics.
Lambda-CDM model and Monthly Notices of the Royal Astronomical Society · Monthly Notices of the Royal Astronomical Society and Universe ·
Neutrino
A neutrino (denoted by the Greek letter ν) is a fermion (an elementary particle with half-integer spin) that interacts only via the weak subatomic force and gravity.
Lambda-CDM model and Neutrino · Neutrino and Universe ·
Parsec
The parsec (symbol: pc) is a unit of length used to measure large distances to astronomical objects outside the Solar System.
Lambda-CDM model and Parsec · Parsec and Universe ·
Physical cosmology
Physical cosmology is the study of the largest-scale structures and dynamics of the Universe and is concerned with fundamental questions about its origin, structure, evolution, and ultimate fate.
Lambda-CDM model and Physical cosmology · Physical cosmology and Universe ·
Planck (spacecraft)
Planck was a space observatory operated by the European Space Agency (ESA) from 2009 to 2013, which mapped the anisotropies of the cosmic microwave background (CMB) at microwave and infra-red frequencies, with high sensitivity and small angular resolution.
Lambda-CDM model and Planck (spacecraft) · Planck (spacecraft) and Universe ·
Quintessence (physics)
In physics, quintessence is a hypothetical form of dark energy, more precisely a scalar field, postulated as an explanation of the observation of an accelerating rate of expansion of the universe.
Lambda-CDM model and Quintessence (physics) · Quintessence (physics) and Universe ·
Redshift
In physics, redshift happens when light or other electromagnetic radiation from an object is increased in wavelength, or shifted to the red end of the spectrum.
Lambda-CDM model and Redshift · Redshift and Universe ·
Reionization
In the field of Big Bang theory, and cosmology, reionization is the process that caused the matter in the universe to reionize after the lapse of the "dark ages".
Lambda-CDM model and Reionization · Reionization and Universe ·
Scale factor (cosmology)
The relative expansion of the universe is parametrized by a dimensionless scale factor a. Also known as the cosmic scale factor or sometimes the Robertson–Walker scale factor, this is a key parameter of the Friedmann equations.
Lambda-CDM model and Scale factor (cosmology) · Scale factor (cosmology) and Universe ·
Shape of the universe
The shape of the universe is the local and global geometry of the universe.
Lambda-CDM model and Shape of the universe · Shape of the universe and Universe ·
Spacetime
In physics, spacetime is any mathematical model that fuses the three dimensions of space and the one dimension of time into a single four-dimensional continuum.
Lambda-CDM model and Spacetime · Spacetime and Universe ·
Standard Model
The Standard Model of particle physics is the theory describing three of the four known fundamental forces (the electromagnetic, weak, and strong interactions, and not including the gravitational force) in the universe, as well as classifying all known elementary particles.
Lambda-CDM model and Standard Model · Standard Model and Universe ·
Theory of everything
A theory of everything (ToE), final theory, ultimate theory, or master theory is a hypothetical single, all-encompassing, coherent theoretical framework of physics that fully explains and links together all physical aspects of the universe.
Lambda-CDM model and Theory of everything · Theory of everything and Universe ·
Vacuum energy
Vacuum energy is an underlying background energy that exists in space throughout the entire Universe.
Lambda-CDM model and Vacuum energy · Universe and Vacuum energy ·
Weak gravitational lensing
While the presence of any mass bends the path of light passing near it, this effect rarely produces the giant arcs and multiple images associated with strong gravitational lensing.
Lambda-CDM model and Weak gravitational lensing · Universe and Weak gravitational lensing ·
Wilkinson Microwave Anisotropy Probe
The Wilkinson Microwave Anisotropy Probe (WMAP), originally known as the Microwave Anisotropy Probe (MAP), was a spacecraft operating from 2001 to 2010 which measured temperature differences across the sky in the cosmic microwave background (CMB) – the radiant heat remaining from the Big Bang.
Lambda-CDM model and Wilkinson Microwave Anisotropy Probe · Universe and Wilkinson Microwave Anisotropy Probe ·
The list above answers the following questions
- What Lambda-CDM model and Universe have in common
- What are the similarities between Lambda-CDM model and Universe
Lambda-CDM model and Universe Comparison
Lambda-CDM model has 88 relations, while Universe has 479. As they have in common 41, the Jaccard index is 7.23% = 41 / (88 + 479).
References
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