Physics Spl

Yes, it's possible to get admission to the M.Sc Physics programme at MJPRU (Mahatma Jyotiba Phule Rohilkhand University) based on your CUET (PG) score, as the university accepts CUET PG scores for admission to PG courses. 

Here's a more detailed breakdown:

CUET PG Acceptance:

MJPRU accepts CUET PG scores for admission to postgraduate (PG) courses, including M.Sc Physics. 

MJPRU Entrance Exam:

MJPRU also conducts its own entrance exam for certain courses, but for courses like BPharm, BTech, MBA, MCA, etc., they accept valid scores of JEE Main, CUET UG & CUET PG entrance exams. 

Eligibility Criteria:

To be eligible for the M.Sc Physics program, you'll need a Bachelor's degree in Physics, Chemistry, and Mathematics with a minimum of 50% marks (or equivalent grade) from a recognised university. 

In Newton's Law of Gravitation, G (Universal Gravitational Constant) has a fixed value as it is a fundamental constant which is:

G determines the strength of gravitational interactions and it remains the same everywhere in the universe. It plays a significant role in cosmology and astrophysics and it is important in calculating the forces between celestial bodies. Due to the gravitational pull of a massive body like Earth, 'g' (Acceleration due to Gravity) is the acceleration which the object experiences. The value of g changes based on the planetary composition, latitude, and altitude. G is universal and g is dependent on the location. This relation can be understood by the following formula:

M represents the mass of the planet, and R is the radius. The concept and its differences help in fields such as space exploration where astronauts experience microgravity in orbit even though the gravitational forces are present.

It is due to a concept taken from Newton's Law of Gravitation. It says that each mass element of the shell puts an attractive force on a particle inside but due to the fact that the shape of the shell is symmetrical, these forces cancel out in every direction.
To prove it mathematically, one can use Gauss's Law for Gravitation. It states that inside a uniformly distributed spherical shell, the net gravitational field is zero. It differs from electrostatics, which states that a conducting shell blocks or stops the external electric fields. The shielding concept is not part of gravitation where the external bodies exert a gravitational force on an object inside the shell. It is the fundamental property of astrophysics and helps in understanding why the gravitational field inside a star or planet depends only on the mass enclosed within a given radius.

Kepler's laws refer to the motion of planets around the Sun and it offers various insights into the celestial mechanics. It includes the following:

• The First Law (Law of Orbits) states that all planets move in elliptical orbits, and the Sun is at one focus. It is against the previous belief that planetary orbits were perfect circles.
• The Second Law (Law of Areas) states the line joining the Sun and a planet sweeps out equal areas in equal time intervals. It means that the planets near to Sun move faster and the ones at more distance, move slower.
• The third Law (Law of Periods) says that the square of a planet's orbital period is directly proportional to the cube of the semi-major axis of its orbit. The mathematical formula is:

According to Newton's Law of Universal Gravitation, each object in the universe attracts every other object with a force that depends on the distance between them and their masses. This force is mathematically given by the following formula:

Here, F is the gravitational force, G is the gravitational constant and m? and m? refers to the masses of the objects, and r represents the distance between them.

Newton's Law of Universal Gravitation explains the behaviour of tides due to the Moon's gravity, planetary motion, and even how satellites orbit the Earth. This law is widely used in space research and astrophysics to find out the masses of the celestial bodies and how they interact with each other. It is accurate in most cases but for extreme gravitational fields, instead of Newton's law, Einstein's General Theory of Relativity is more useful.

Students who wish to study offline can download the NCERT Class 12 Physics Chapter 12 Atoms PDF from Shiksha's homepage or other educational platforms. This allows students to access NCERT Solutions PDFs anytime without an internet connection. 

NCERT Solution Class 12 Physics Ch 12 Atoms PDF: Download Free PDF

The PDF provides a detailed explanations along with solved numerical problems, and conceptual insights to help students revise and prepare better. By downloading the PDF, students can practice various types of theoretical and numerical questions, which improve their problem-solving skills and boosts their exam performance.

Class 12 Physics Ch 12 Atoms NCERT Solutions covers various important topics that play a significant role in modern physics. Here are some of the topics students must include during their exam preparation:

• Rutherford's Atomic Model

• Bohr's Model of the Hydrogen Atom

• Energy Quantization

• The Hydrogen Spectral Series (Lyman, Balmer, Paschen, Brackett, and Pfund series)

• de Broglie's Explanation of Bohr's Second Postulate

• The Limitations of Bohr's Model. 

Additionally, it also includes X-ray Spectra and Moseley's Law, which help explain the relationship between atomic number and X-ray frequency. These concepts are frequently asked in board exams and entrance exams like JEE and NEET.

NCERT Solutions for Class 12 Physics Chapter 12 Atoms are important for students preparing for CBSE board exams as well as competitive exams like JEE and NEET. 

Class 12 Physics Chapter 12 Atoms conisists of fundamental concepts such as Hydrogen Spectral Series, Rutherford's Atomic Theory, Bohr's Model, and Energy Quantization. Being aware of these concepts will prepare students build a strong foundation in modern physics, which is important for advanced studies in engineering and medical fields. The NCERT solutions pdfs also provide step-by-step problem-solving methods, making it easier for students to tackle with numerical and theoretical questions in a much better way.