In economics, inflation is a rise in the general level of prices of goods and services in an economy over a period of time. When the general price level rises, each unit of currency buys fewer goods and services. Consequently, inflation also reflects an erosion in the purchasing power of money – a loss of real value in the internal medium of exchange and unit of account in the economy. A chief measure of price inflation is the inflation rate, the annualized percentage change in a general price index (normally the Consumer Price Index) over time.
Inflation's effects on an economy are various and can be simultaneously positive and negative. Negative effects of inflation include a decrease in the real value of money and other monetary items over time, uncertainty over future inflation which may discourage investment and savings, and if inflation is rapid enough, shortages of goods as consumers begin hoarding out of concern that prices will increase in the future. Positive effects include ensuring central banks can adjust nominal interest rates (intended to mitigate recessions), and encouraging investment in non-monetary capital projects.
Milton Friedman (July 31, 1912 – November 16, 2006) was an American economist, statistician, and author who taught at the University of Chicago for more than three decades. He was a recipient of the Nobel Memorial Prize in Economic Sciences, and is known for his research on consumption analysis, monetary history and theory, and the complexity of stabilization policy. As a leader of the Chicago school of economics, he influenced the research agenda of the economics profession. A survey of economists ranked Friedman as the second most popular economist of the twentieth century behind John Maynard Keynes, and The Economist described him as "the most influential economist of the second half of the 20th century…possibly of all of it."
Friedman's challenges to what he later called "naive Keynesian" (as opposed to New Keynesian) theory began with his 1950s reinterpretation of the consumption function, and he became the main advocate opposing activist Keynesian government policies. In the late 1960s he described his own approach (along with all of mainstream economics) as using "Keynesian language and apparatus" yet rejecting its "initial" conclusions. During the 1960s he promoted an alternative macroeconomic policy known as "monetarism". He theorized there existed a "natural" rate of unemployment, and argued that governments could increase employment above this rate (e.g., by increasing aggregate demand) only at the risk of causing inflation to accelerate. He argued that the Phillips curve was not stable and predicted what would come to be known as stagflation. Friedman argued that, given the existence of the Federal Reserve, a constant small expansion of the money supply was the only wise policy.
Leonard Susskind (born 1940) is the Felix Bloch Professor of Theoretical Physics at Stanford University. His research interests include string theory, quantum field theory, quantum statistical mechanics and quantum cosmology. He is a member of the National Academy of Sciences, and the American Academy of Arts and Sciences, an associate member of the faculty of Canada's Perimeter Institute for Theoretical Physics, and a distinguished professor of the Korea Institute for Advanced Study.
Susskind is widely regarded as one of the fathers of string theory, having, with Yoichiro Nambu and Holger Bech Nielsen, independently introduced the idea that particles could in fact be states of excitation of a relativistic string. He was the first to introduce the idea of the string theory landscape in 2003.
In 1997, Susskind was awarded the J.J. Sakurai Prize for his "pioneering contributions to hadronic string models, lattice gauge theories, quantum chromodynamics, and dynamical symmetry breaking." Susskind's hallmark, according to colleagues, has been the application of "brilliant imagination and originality to the theoretical study of the nature of the elementary particles and forces that make up the physical world."
What is Inflation?
What is Inflation
What is Inflation?
Inflation einfach erklärt (by explainity®)
Inflation and Bubbles and Tulips: Crash Course Economics #7
Milton Friedman - Understanding Inflation
Econ Vids for Kids: What is Inflation?
Inflation
What Causes Inflation?
Michael Snyder- Deflation then Inflation Through the Roof
Der Euro fällt immer mehr - Deutschlands Inflation 2016 - Dokumentation 2015 Neu in HD
Inflation and its Causes
Aspects of Eternal Inflation, Lecture 1 of 4 | Leonard Susskind
inflation part 1
What is Inflation?
What is Inflation
What is Inflation?
Inflation einfach erklärt (by explainity®)
Inflation and Bubbles and Tulips: Crash Course Economics #7
Milton Friedman - Understanding Inflation
Econ Vids for Kids: What is Inflation?
Inflation
What Causes Inflation?
Michael Snyder- Deflation then Inflation Through the Roof
Der Euro fällt immer mehr - Deutschlands Inflation 2016 - Dokumentation 2015 Neu in HD
Inflation and its Causes
Aspects of Eternal Inflation, Lecture 1 of 4 | Leonard Susskind
inflation part 1
World Events Mean Deflation First, Then Inflation
Explaining Inflation | by Wall Street Survivor
Crash Course: Chapter 10 - Inflation by Chris Martenson
EconMovies 6: Back to the Future (Nominal vs. Real, Unemployment, Inflation)
16. Qu'est-ce que l'inflation ?
BambiBlaze Body Inflation: Dr. Blimp 7
Inflation Commercials
Princess Maydine's Blueberry inflation (Extended Version)
Gravitational Wave Discovery! Evidence of Cosmic Inflation
Painless
So easy
You come fast
And leave me
Half a life
For one kiss
Inflation
And now this
The player game
Innocently
Was always there
But used to be
Only one way
To feel love
But now it is