Uploaded August 2022 | Updated September 2026, 1 week ago
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Bremsstrahlung is the electromagnetic radiation emitted in the form of photons when a charged particle is decelerated upon striking against another charged particle. This radiation gives a continuous X-ray spectrum. This is also known as “braking radiation”. These charged particles are mainly electrons and atomic nuclei of metals. Let us now study bremsstrahlung radiation, its causes, and effects.
In the classical explanation of bremsstrahlung radiation, the quantum effects are neglected and a comparatively simpler approach was considered by Larmor. Bremsstrahlung has its uses in radiation safety equipment and astrophysics. Bremsstrahlung radiation is often considered to be secondary radiation.
Bremsstrahlung Radiation
Bremsstrahlung radiation is a type of electromagnetic radiation emitted when a charged particle upon getting deflected by another charged particle is decelerated. These charged particles are mainly electrons or atomic nuclei. The particles in motion upon clashing lose kinetic energy. The lost energy is emitted as radiation in the form of photons. Thus the law of conservation of energy is also satisfied. This is known as the bremsstrahlung radiation. This bremsstrahlung radiation gives a continuous spectrum. The peak intensities tend to shift towards higher frequencies with the increase in the energy of the decelerated charged articles. This is the bremsstrahlung radiation definition. Bremsstrahlung radiation is of two types namely inner bremsstrahlung and outer bremsstrahlung radiation. We’ll be discussing this later in this article.
Causes of Bremsstrahlung Radiation
Bremsstrahlung can be defined as a process by which some of the energy of the celestial rays is scattered into the atmosphere of Earth. The chromosphere emits solar x-rays in the form of bremsstrahlung radiation. This is generated by fast-moving electrons. However internal bremsstrahlung takes place in case of radioactive disintegration. During beta decay which involves the emission of electrons and positrons, the clash between these charged particles results in the emission of bremsstrahlung radiation. It is mainly caused by the acceleration and deceleration of charged particles such as atomic nuclei and electrons. If the particles emit bremsstrahlung radiation while being accelerated by an external magnetic field it is also known as synchrotron radiation.
Bremsstrahlung X- Rays
The bremsstrahlung x-rays are emitted when electrons get decelerated when fired against a metal target. These charged particles emit bremsstrahlung radiation in the form of photons or bremsstrahlung x-rays. The continuous spectrum formed due to the bombardment of electrons lies in the x-ray region of the electromagnetic spectrum. The energy peaks of the x-ray spectrum tend to shift towards higher frequencies with the increase in energy of the electrons. Often the bombarding electrons also eject electrons from the inner atomic shells of the target metal. The vacancies are quickly filled by dropping electrons from the higher atomic shells. As a result, bremsstrahlung x-rays are emitted.
Inner and Outer Bremsstrahlung
Inner bremsstrahlung and outer bremsstrahlung are the two types of bremsstrahlung radiations. The inner bremsstrahlung is also known as internal bremsstrahlung is caused by the electrons emitted from a radioactive decaying nucleus. This is a feature of beta decay in the nuclei. However, the outer bremsstrahlung is caused when electrons emitted from a separated nucleus are bombarded on other nuclei. The bremsstrahlung decreases constantly with the increase in the energy of the beta particles in the case of electrons and positrons which are emitted by the electron-nuclei pair in case of beta decay. The bremsstrahlung is emitted in case of electron capture without emission of any charged particle. Electron capture requires the energy of a neutrino. The bremsstrahlung radiation is the result of the acceleration of the captured electrons. These types of radiations often have the same frequencies as gamma radiation. These radiations do not exhibit any spectral lines of the gamma radiation and hence can not be considered as gamma decay.
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Bremsstrahlung is the electromagnetic radiation emitted in the form of photons when a charged particle is decelerated upon striking against another charged particle. This radiation gives a continuous X-ray spectrum. This is also known as “braking radiation”. These charged particles are mainly electrons and atomic nuclei of metals. Let us now study bremsstrahlung radiation, its causes, and effects.
In the classical explanation of bremsstrahlung radiation, the quantum effects are neglected and a comparatively simpler approach was considered by Larmor. Bremsstrahlung has its uses in radiation safety equipment and astrophysics. Bremsstrahlung radiation is often considered to be secondary radiation.
Bremsstrahlung Radiation
Bremsstrahlung radiation is a type of electromagnetic radiation emitted when a charged particle upon getting deflected by another charged particle is decelerated. These charged particles are mainly electrons or atomic nuclei. The particles in motion upon clashing lose kinetic energy. The lost energy is emitted as radiation in the form of photons. Thus the law of conservation of energy is also satisfied. This is known as the bremsstrahlung radiation. This bremsstrahlung radiation gives a continuous spectrum. The peak intensities tend to shift towards higher frequencies with the increase in the energy of the decelerated charged articles. This is the bremsstrahlung radiation definition. Bremsstrahlung radiation is of two types namely inner bremsstrahlung and outer bremsstrahlung radiation. We’ll be discussing this later in this article.
Causes of Bremsstrahlung Radiation
Bremsstrahlung can be defined as a process by which some of the energy of the celestial rays is scattered into the atmosphere of Earth. The chromosphere emits solar x-rays in the form of bremsstrahlung radiation. This is generated by fast-moving electrons. However internal bremsstrahlung takes place in case of radioactive disintegration. During beta decay which involves the emission of electrons and positrons, the clash between these charged particles results in the emission of bremsstrahlung radiation. It is mainly caused by the acceleration and deceleration of charged particles such as atomic nuclei and electrons. If the particles emit bremsstrahlung radiation while being accelerated by an external magnetic field it is also known as synchrotron radiation.
Bremsstrahlung X- Rays
The bremsstrahlung x-rays are emitted when electrons get decelerated when fired against a metal target. These charged particles emit bremsstrahlung radiation in the form of photons or bremsstrahlung x-rays. The continuous spectrum formed due to the bombardment of electrons lies in the x-ray region of the electromagnetic spectrum. The energy peaks of the x-ray spectrum tend to shift towards higher frequencies with the increase in energy of the electrons. Often the bombarding electrons also eject electrons from the inner atomic shells of the target metal. The vacancies are quickly filled by dropping electrons from the higher atomic shells. As a result, bremsstrahlung x-rays are emitted.
Inner and Outer Bremsstrahlung
Inner bremsstrahlung and outer bremsstrahlung are the two types of bremsstrahlung radiations. The inner bremsstrahlung is also known as internal bremsstrahlung is caused by the electrons emitted from a radioactive decaying nucleus. This is a feature of beta decay in the nuclei. However, the outer bremsstrahlung is caused when electrons emitted from a separated nucleus are bombarded on other nuclei. The bremsstrahlung decreases constantly with the increase in the energy of the beta particles in the case of electrons and positrons which are emitted by the electron-nuclei pair in case of beta decay. The bremsstrahlung is emitted in case of electron capture without emission of any charged particle. Electron capture requires the energy of a neutrino. The bremsstrahlung radiation is the result of the acceleration of the captured electrons. These types of radiations often have the same frequencies as gamma radiation. These radiations do not exhibit any spectral lines of the gamma radiation and hence can not be considered as gamma decay.

![Space Part 1 - Orbital Speed (IGCSE 0625/0972)
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The topic space is the newly injected topic in 0625/0972 IGCSE physics curriculum, exam will be conducted from 2023 onwards
Important Definition
Define Rotation of Earth: The circular movement of the Earth about its own axis is called as the rotation of the Earth.
Define Average orbital speed: It is defined using the equation: v = 2??r /T where r is the average radius of the orbit and T is the orbital period
Define Solar system: Solar system is a single term that includes eight planets and their moons in orbit round the sun. Also included in the solar system are the smaller bodies such as the comets., asteroids, and the meteoroids.
Define Orbital distance: Orbital distance is the term that tells us the time taken by one object to revolve around the other.
Define Orbital duration[ Orbital time}: Orbital duration is the time taken by one object to completely orbit around the other.
Define gravitational field strength: Gravitational field strength is a term that indicates the amount of gravitational force that is exerted per unit mass at a particular point. It has a symbol g
Define Interstellar clouds of gas and dust: It is a cloud comprising of dust, plasma and gases present in all the galaxies, including our own.
Define accretion disc: These are structures that surround the celestial objects such as the stars and the black holes. These structures are made of gas, plasma and dust
Define Planetary data: It refers to the data that gives us information on the different planets based on researches and explorations
6.2 Stars and the Universe
Define Stars: Stars are massive , self-luminous celestial objects, made of Hydrogen and Helium
Define Proto stars: A Protostar is a young star. .It is formed as a result of accretion in the nebula.
Define Stable stars: In every star, there is the gas pressure that exerts an outward force from the centre and at the same time , there is gravity that is pulling the atoms of Hydrogen and Helium inwards. When the outward pushing force balances the gravitational force, we call the star as a stable tar. Example of a stable star is the Sun.
Define Sun: The Sun is a very bright, luminous, celestial and a stable star, situated in the spiral arm of the Milky Way galaxy and at the centre of the Solar System.
Define Galaxy: The word galaxy encompasses billions of stars along with their solar systems, gas and dust held by their gravity. There are more than a hundred billion galaxies in the universe.
Define Milky way: Milky way is a spiral galaxy that includes our solar system. It has billions of stars, including our Sun.
Define Universe: Universe refers to the space, time and matter and all the laws that govern them.
Define Light-year: One light-year is the distance traveled in (the vacuum of) space by light in one year.
Define Red giants: These are massive , luminous stars with a very low surface temperature and a high volume , with a reddish-orange hue, in their final stage of stellar evolution and that have exhausted their supply of Hydrogen in their core. Examples: Aldebaran (Alpha Tauri) and Mira (Omicron Ceti).
Define Red supergiants: Red supergiants are aging giant stars with a minimum of 15 solar masses. [solar mass refers to the mass of the sun, when used as a unit of mass. One solar mass is equal to 1.989 x 1030 kg ]
Define Supernova: Supernova is a powerful and luminous stellar explosion, that happens when a star has reached the end of its life. Example: Keplers Supernova
Define Nebula: Nebula is a Latin word for fog or cloud. It consists of interstellar clouds consisting of Helium, Cosmic Dust, ionized gases, hydrogen as well as molecular clouds. [There are in all 5 different types of Nebulae, namely; emission nebulae, reflection nebulae, dark nebulae, planetary nebulae, and supernova remnants.
Define Black hole: A black hole is a region in the space, in which the effect of gravity is so strong, that it lets nothing escape out f it, not even light. The region appears to be black and circular.[ There are approximately 100 billion super massive black holes]
Define Redshift: Redshift is a phenomenon in which the spectrum of an astronomical object gets displaced towards the longer( red) wavelength.
Define Cosmic microwave background radiation (CMBR): Cosmic microwave background radiation (CMBR) is the leftover of the cosmic radiation after the big bang.
Define Hubble constant Ho: Hubble constant is the ratio of the speed at which the galaxy is moving away from the Earth to its distance from the Earth Space Part 1 - Orbital Speed (IGCSE 0625/0972)](https://i.ytimg.com/vi/xT_XJeoeuAw/mqdefault.jpg)



