Lohith will gives a brief overview of what electromagnetic radiation is all about.
About the speaker:
Lohith is 14 years old and is a part of Mango Astronomy club. He is passionate about physics.
3. Schlumberger-Private
Intro
▪ It is nothing but a form of energy travelling in the form electric and
magnetic waves moving simultaneously.
▪ It is the second strongest force out of the four.
4. Schlumberger-Private
Electromagnetic
Spectrum
• It is a wide range of lights of different wavelengths.
• A spectrum is literally limitless and as the frequency increases
the energy of the photon increases proportionally.
5. Schlumberger-Private
Photo
ns
• Photons are the particles of light.
• Photon is actually a wavicle.
• Different frequency photons exhibit different types of light In
the electromagnetic spectrum.
6. Schlumberger-Private
Photoelectric effect
• It is the famous theory for which Albert Einstein got awarded
with the Noble Prize.
• It says that when light(generally UV) is shone on a metal it
emits electrons.
• This theory helped in the wave-particle duality.
8. Schlumberger-Private
Cosmic Microwave
Background
• CMB is the Electromagnetic remnant of the Big Bang.
• The intense high frequency radiation got red shifted into
microwaves.
• The recording of CMB in the sky has led to the creation of the
universal map using the Wilkinson Microwave Anisotropy
Probe.
9. Schlumberger-Private
Doppler
Effect
• Doppler effect is a phenomenon found in waves when their
origins move very fast towards or away from the receiver.
• If the origin moves towards the receiver then the waves get
compressed reducing the wavelength resulting in increase in
the frequency called Blue-Shift.
• If the origin moves away from the receiver then the waves get
expanded increasing the wavelength resulting in reduction in
the frequency called Red-Shift.
• Example of such phenomena:
11. Schlumberger-Private
Cherenkov
Radiation
• Light is the fastest thing in vacuum and its speed is called the
cosmic speed limit but certain particles are faster than light in
other mediums.
• Electron is faster than light in D2O i.e Heavy Water. So as electron
also emits and reflects light, it is an origin of light waves. This results
in total compression of waves in front of the electron due to
doppler effect.
• This emits an different type of radiation called Cherenkov radiation.
13. Schlumberger-Private
LASERS
• LASER-Light Amplification by Stimulated Emission of Radiation.
• Laser is nothing but emitting an amplified and focused
single-frequency beam of light.
• The general absorption and emission of light by an atom is
called spontaneous emission of light.
• Whereas stimulated emission of radiation is about emitting a
photon in the presence of a another one which is similar to this in
the means of frequency,amplitude,phase,polarization.
14. Schlumberger-Private
LASERS
• For this the electron in the excited state should pause at its
metastable state non-radiatively and then further cascade to
its ground state.
15. Schlumberger-Private
Yarkovsky
Effect
• This is the key to the human race for quick transportation of
tiny probes to another star system.
• This is the propulsion of objects using momentum of light when
an object’s surface heats up, it gains energy and it cools down by
emitting photons, this helps in its propulsion.
• In future there is a plan of sending tiny chips with lenseless
cameras to Alpha centauri at 20% the speed of light.
17. Schlumberger-Private
Rayleigh
effect• The sky’s blue colour and blood moon’s red colour all has a
reason that is nothing but Rayleigh effect.
• The blue colour gets scattered in the sky giving its colour an
blocking this wavelength from reaching eclipsed moon.
•This is called the “Blood moon effect”.
18. Schlumberger-Private
Absorption and emission of
light
• Light interacts with an atom by exciting the an electron and pushing
it to a higher orbit.
• The excited electron again returns back to its ground or mean state
by emitting a photon.
19. Schlumberger-Private
Absorption and emission
spectrum
• Few elements absorb certain wavelengths of light and emit them.
• So certain colours of the Total spectrum won’t be visible. And they will
be emitted while the electrons of the element return to their ground
states.
• The band of colours obtained after absorption is called absorption
spectrum and the one obtained on emission is called emission spectrum.
• Each element has its own spectrum.
• When white light passes through a planet’s atmosphere, the elements
absorb certain wavelengths through which we can find out the
atmospheric composition.
21. Schlumberger-Private
Virtual
Photons
• Virtual photons are simple photon like disturbance in
the electromagnetic ield.
• An real photon is a real thing that has an inluence on quantum
electromagnetic ield and is stronger and much longer than virtual
disturbances.
• These virtual photons are the actual medium of
Electromagnetic force.
22. Schlumberger-Private
Epoch of
reionisation
• The early universe was small and illed with hydrogen atoms.
• These atoms didn’t allow light to pass through them leaving the
universe dark.
• With the formation of the irst galaxies the hydrogen atoms started to
get illed up with energy leaving no space for more this paved up the
way for the irst photon to travel out of the huge cloud into free space.
• The period during which this event occurred is called the epoch
of reionisation.
• Astronomers cannot see any incident that occurred before
this reionisation through electromagnetic techniques like
telescopes.