# Complete Spotlights

## Special relativity

### Einstein’s Nobel heritage

An overview of Nobel prizes connected with relativistic physics

### Is the whole the sum of its parts?

Why Einstein’s famous formula tells us that the whole, as far as mass is concerned, is often less than the sum of its parts

### The definition of “now”

Why it is necessary to define simultaneity, and how best to go about defining it.

### Waves, motion and frequency: the Doppler effect

How motion influences waves, or other kinds of ever-repeating signals, in classical physics and in special relativity.

### From E=mc² to the atomic bomb

The subtle connections between Einstein’s formula, nuclear fission and nuclear fusion

### The dialectic of relativity

How relativity can reconcile statements that, at first glance, appear to be contradictory

### Time dilation on the road

How you can picture the relativity of simultaneity and time dilation, using a simple geometric analogy

### The case of the travelling twins

Why the so-called “twin paradox” isn’t really a paradox

### Twins on the road

How one can picture the situation of the travelling twin, using a simple geometric analogy

## General relativity

### Einstein’s Nobel heritage

An overview of Nobel prizes connected with relativistic physics

### Measuring light deflection with radio telescopes

Very long baseline interferometry (VLBI) can be used to measure deflection of light by the sun with very high accuracy, which allows the testing of a prediction of general relativity.

### The Singularity Theorem (Nobel Prize in Physics 2020)

In 2020, Roger Penrose was awarded half of the Nobel prize in physics for proving that black hole formation is a robust prediction of Einstein’s general theory of relativity.

### From soap bubbles to Einstein

Most readers will know them from childhood: soap bubbles

### Gravitational deflection of light

On one of the fundamental consequences of general relativity: the deflection of light by gravity

### Mass and more

An account of which physical properties act as sources of gravity – includes consequences for collapsing stars and for cosmology

### Spacetime singularities

Information about the most disturbing feature of Einstein’s theory – ragged edges of spacetime known as singularities.

### The elevator, the rocket, and gravity: the equivalence principle

Information about the principle that Einstein took as a starting point for developing his general theory of relativity

### The realm of relativistic hydrodynamics

Modeling relativistic fluids and the phenomena associated with them – from supernovae and jets to merging neutron stars

### Varying Newton’s constant: A personal history of scalar-tensor theories

Information about a modification of Einstein’s theory of general relativity in which the gravitational constant is not a constant.

### Gravity: from weightlessness to curvature

So what is gravity in Einstein’s theory? The answer: in part, an illusion; in part, an aspect of geometry.

### Of singularities and breadmaking

About some characteristic properties of spacetime near singularities – and the violent deformations they cause for any object unlucky enough to approach a singularity

### The equivalence principle and the deflection of light

The connection between one of the fundamental principles of general relativity and the gravitational deflection of light

### The gravity of gravity

An important property of gravity in Einstein’s theory is that it can create more gravity. The result is “non-linearity” – the gravitational influence of two bodies isn’t just the sum of their separate influences!

### The many ways of building an empty, unchanging universe

More information on one particular answer to the question of how much variety is permitted in general relativity – how many ways are there of constructing a universe that is completely empty of all matter?

## Gravitational waves

### Gravitational wave detectors find 56 potential cosmic collisions

During collaborative measurement campaigns, so-called observation runs, the worldwide gravitational wave detector network listens for signals from space. During the third observation run “O3”, which started on April 1st, 2019, the LIGO detectors (USA), Virgo (Italy), and GEO600 (Germany) recorded a range of promising signals.

### Of gravitational waves and spherical chickens

Information about a class of simple model universes, each an expanding cosmos filled with gravitational waves

### The wave nature of simple gravitational waves

A closer look at the way that simple gravitational waves propagate through space with time

### Listening posts around the globe

Overview of the gravitational wave detectors currently operational, or under construction

### Einstein@Home – gravitational waves for everybody

Information on how you personally can help with the search for gravitational wave – by donating processing time on your private computer

### Catching the wave with light

Some information on how interferometric detectors such as LIGO or GEO600 work

### Small vibrations

Some information on how the vintage models among gravitational wave detectors work – resonant detectors

### LISA – Hunting waves in space

Information about the latest version of the most ambitious gravitational wave project – a detector in space

### Chirping neutron stars

For some gravitational wave signals, one can go beyond graphs and animations – they can be made audible

### Observation of Gravitational Waves from a Binary Black Hole Merger

Albert Einstein predicted their existence back in 1916, and on 14 September 2015 they were directly detected for the first time: Gravitational waves. Two large interferometric detectors of the LIGO Scientific Collaboration with major contributions from German researchers detected the signal known as “GW150914”. The waves originate from the merger of two black holes and are the first direct observation of these exotic objects.

### White Dwarf binaries as gravitational wave sources

White Dwarf binaries, their properties, and the role they will play for the planned space-borne gravitational wave detector LISA.

## Black Holes & Co.

### The Singularity Theorem (Nobel Prize in Physics 2020)

In 2020, Roger Penrose was awarded half of the Nobel prize in physics for proving that black hole formation is a robust prediction of Einstein’s general theory of relativity.

### Descent into a black hole

The story of an expedition’s closer and closer approach to a black hole – too close?

### How many different kinds of black holes are there?

Once they have settled down, there are actually only very few different kinds of black hole – find out which, and how black holes shed other distinguishing marks.

### What figure skaters, orbiting planets and neutron stars have in common

Some information about what is called the conservation of angular momentum, and its consequences for neutron stars, black holes and the matter disks around them

### Heat that meets the eye

The connection between temperature and the emission of electromagnetic radiation, as well as the consequences for stars, matter disks around black holes, and cosmology

### Luminous disks: How black holes light up their surroundings

How the fact that black holes are very efficient in attracting surrounding matter leads to some of the most spectacularly luminous phenomena in the whole of the cosmos

### Active black holes: Ultra-hot cosmic beacons

What astronomers can see once a black hole has heated up its cosmic neighbourhood, stimulating it to emit bright radiation

### Changing places – space and time inside a black hole

How, in one sense, space and time switch their roles inside a black hole – and why this leads to a black hole’s most characteristic property, namely that nothing can get out

### Particle accelerators as black hole factories?

The intriguing possibility that the next generation of particle accelerators might produce – and allow the detection of – miniature black holes

### The dark heart of the Milky Way

Information about the closest supermassive black hole – the central object of our own galaxy

## Cosmology

### A tale of two big bangs

In cosmology, “big bang” has two different meanings – and if you want to understand what’s going on, you should be aware of that difference.

### Big Bang Nucleosynthesis: Cooking up the first light elements

How the first nuclei of helium, lithium and other light elements were cooked up shortly after the big bang

### Cosmic Sound: Curvature and the cosmic background radiation

How the spatial geometry of the universe can be derived by observing the cosmic background radiation

### Searching for the quantum beginning of the universe

About attempts to understand the beginning of our universe using different approaches to quantum gravity

### Avoiding the big bang

The collapsing and then re-expanding quantum universe that loop quantum gravity offers as a replacement of the standard big bang models

### Equilibrium and Change: The physics behind Big Bang Nucleosynthesis

The physics behind Big Bang Nucleosynthesis, the period shortly after the big bang that saw the first production of light elements such as helium and lithium

### Heat that meets the eye

The connection between temperature and the emission of electromagnetic radiation, as well as the consequences for stars, matter disks around black holes, and cosmology

### The shape of space

The different space geometries allowed by the big bang models – do we live on a hypersphere?

### Elements of the past: Big Bang Nucleosynthesis and observation

How to reconstruct the abundances of light elements shortly after the big bang, and thus test some important predictions of the big bang models against observation

### Taming infinity with loops

How loop quantum gravity could replace the absurd state of infinite density, the big bang with which, according to Einstein’s relativity, the universe began

### The mathematical universe

Why cosmology is not only a matter for astronomers and physicists, but also for mathematicians

## Relativity and the Quantum

### The sum over all possibilities: The path integral formulation of quantum theory

About the path integral approach to quantum theory

### Actors on a changing stage: quantum gravity and background independence

The principle of background independence – space and time are no fixed structure, but take part in the dynamical evolution of the world – and its consequences for the problem of quantum gravity

### Extra dimensions – and how to hide them

Why our universe could possess dimensions beyond length, width and depth – and why those dimensions need not be noticeable in everyday life

### Searching for the quantum beginning of the universe

About attempts to understand the beginning of our universe using different approaches to quantum gravity

### Avoiding the big bang

The collapsing and then re-expanding quantum universe that loop quantum gravity offers as a replacement of the standard big bang models

### Geometry from order: causal sets

An overview of the causal set approach to a theory of quantum gravity

### The embedded universe

Is our three-dimensional world embedded in a higher-dimensional space?

### Particle accelerators as black hole factories?

The intriguing possibility that the next generation of particle accelerators might produce – and allow the detection of – miniature black holes

### Taming infinity with loops

How loop quantum gravity could replace the absurd state of infinite density, the big bang with which, according to Einstein’s relativity, the universe began

### Hunting for extra dimensions

Ways of detecting extra dimensions – and why the fact that our earth orbits the sun is a relevant data point

### Simplicity in higher dimensions

Why matters that seem rather complicated might be much more simple in higher dimensions

### The fabric of space: spin networks

The quantum structure of space according to loop quantum gravity