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Flatness problem and Planck units

Shortcuts: Differences, Similarities, Jaccard Similarity Coefficient, References.

Difference between Flatness problem and Planck units

Flatness problem vs. Planck units

The flatness problem (also known as the oldness problem) is a cosmological fine-tuning problem within the Big Bang model of the universe. In particle physics and physical cosmology, Planck units are a set of units of measurement defined exclusively in terms of five universal physical constants, in such a manner that these five physical constants take on the numerical value of 1 when expressed in terms of these units.

Similarities between Flatness problem and Planck units

Flatness problem and Planck units have 15 things in common (in Unionpedia): Age of the universe, Big Bang, Cosmic microwave background, Cosmic time, Cosmological constant, Einstein field equations, Friedmann equations, General relativity, Gravitational constant, Hubble's law, Mass–energy equivalence, Physical cosmology, Planck units, Speed of light, Stephen Hawking.

Age of the universe

In physical cosmology, the age of the universe is the time elapsed since the Big Bang.

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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.

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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.

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Cosmic time

Cosmic time (also known as time since the big bang) is the time coordinate commonly used in the Big Bang models of physical cosmology.

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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.

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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.

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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.

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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.

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Gravitational constant

The gravitational constant (also known as the "universal gravitational constant", the "Newtonian constant of gravitation", or the "Cavendish gravitational constant"), denoted by the letter, is an empirical physical constant involved in the calculation of gravitational effects in Sir Isaac Newton's law of universal gravitation and in Albert Einstein's general theory of relativity.

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Hubble's law

Hubble's law is the name for the observation in physical cosmology that.

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Mass–energy equivalence

In physics, mass–energy equivalence states that anything having mass has an equivalent amount of energy and vice versa, with these fundamental quantities directly relating to one another by Albert Einstein's famous formula: E.

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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.

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Planck units

In particle physics and physical cosmology, Planck units are a set of units of measurement defined exclusively in terms of five universal physical constants, in such a manner that these five physical constants take on the numerical value of 1 when expressed in terms of these units.

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Speed of light

The speed of light in vacuum, commonly denoted, is a universal physical constant important in many areas of physics.

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Stephen Hawking

Stephen William Hawking (8 January 1942 – 14 March 2018) was an English theoretical physicist, cosmologist, and author, who was director of research at the Centre for Theoretical Cosmology at the University of Cambridge at the time of his death.

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The list above answers the following questions

Flatness problem and Planck units Comparison

Flatness problem has 69 relations, while Planck units has 207. As they have in common 15, the Jaccard index is 5.43% = 15 / (69 + 207).

References

This article shows the relationship between Flatness problem and Planck units. To access each article from which the information was extracted, please visit:

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