- Isaac Newton developed his law of universal gravitation in the late 17th century, stating that every particle in the universe attracts every other particle with a force directly proportional to their masses and inversely proportional to the square of the distance between them.
- Albert Einstein's theory of general relativity, published in 1915, revolutionized the understanding of gravity by describing it as the curvature of space-time caused by mass and energy, providing a new framework for how gravity behaves in extreme conditions.
- According to Einstein's theory, massive objects warp the fabric of space-time around them, creating what we perceive as gravity - objects with mass and energy tell space-time how to curve, and the curved space-time
Critique Paper Example Short Story - Article CritiquGladys Cepparulo
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Here are some of the key challenges a psychotherapist may face when working with clients who self-harm or have eating disorders:
- Building trust and rapport. Clients may be reluctant to open up about their behaviors and underlying issues due to shame, guilt or fear of judgment. The therapist must create a safe, non-judgmental space to facilitate open communication.
- Addressing underlying causes. Self-harm and disordered eating are usually coping mechanisms for deeper emotional or psychological pain. The therapist needs to help the client gain insight into triggers and root causes like trauma, low self-esteem, perfectionism, etc.
- Managing risk of harm. The therapist is responsible for ensuring the client's safety and reducing risk
Project work plan and budget matrix cp 2016LemardeGuia
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This document provides a project work plan and budget matrix for a Child Protection Policy at a school. The objectives are to create a safe learning environment and address irresponsible behavior by 45 out of 100 students. Activities include developing child rights policies, student profiling, orientations, a film viewing, building a child protection center and park, and seminars on basic laws. The activities will be conducted between April 2016 and October 2016. Most have budgets between P500-P5500 from MOOE funds to cover expenses like tarps, snacks, and certificates. The coordinator and school head are responsible for implementation.
This certificate of recognition from Bugwak Elementary School recognizes an academic achiever for the first quarter of the 2019-2020 school year. It was issued on September 6, 2019 and signed by Vanessa Williams as both the class adviser and school head. The certificate commends the student's achievement and effort during the specified time period.
The document outlines guidelines for administering a regional unified numeracy test in DepEd Region VIII. It aims to assess learners' competencies in the four fundamental math operations (addition, subtraction, multiplication, division) from grades 3 to 10. Teachers must give the 10-12 item test within 10-15 minutes depending on grade level. They are responsible for orientation, administration, scoring, and reporting results. Learners are categorized as highly numerate, moderately numerate, or non-numerate based on their scores. Identified non-numerates must receive intervention through additional testing and enrichment activities. Monitoring and evaluation of the test is done by CID Chiefs, Supervisors and other personnel.
The Civic Welfare Training and Service Module is designed to equip individuals with the knowledge and skills necessary for active participation in community development. Through a comprehensive curriculum, participants engage in theoretical and practical aspects of civic responsibilities, social issues, and community outreach. This module aims to foster a sense of social responsibility and empower participants to contribute meaningfully to the well-being of society through various service initiatives.
The Bambang Elementary School in Pasig City has created a School Action Plan for its Supreme Pupil Government (SPG) for the 2018-2019 school year. The plan outlines activities for each month from May to March focused on cleanliness drives, celebrations, campaigns, and meetings. Key events include Brigada Eskwela in May, a Friendship Day in June, various celebrations and campaigns throughout the year, and the induction of new SPG officers in March. The plan aims to promote student leadership and involvement in bettering the school.
This document discusses RPMS tools and performance indicators for teachers in the Philippines. It explains that there are two RPMS tools for different levels of teachers that assess them on key result areas, objectives, means of verification, and performance indicators. It provides examples of how a Teacher I and Master Teacher I would be assessed and rated using their submitted means of verification for various objectives. Sample scenarios show the teacher's quality and efficiency ratings, average rating, and overall score. The document aims to help teachers and evaluators understand how to use the RPMS tools and what documentation to include for assessment.
Gravitation, free fall, variation in 'g' and keplers law lecture wiseRohan Jain
?
This document contains lecture notes on gravitational force and Newton's law of universal gravitation. It discusses key topics including:
- Gravitational force is a fundamental force that attracts all objects with mass. Newton's law of gravitation describes the force as directly proportional to the product of the masses and inversely proportional to the square of the distance between them.
- Kepler's laws of planetary motion describe how planets move in elliptical orbits with the sun at one focus. Kepler's first law states orbits are ellipses, the second that planets sweep out equal areas in equal times, and the third relates orbital periods to orbital radii.
- The value of the gravitational acceleration g varies depending on location, altitude,
1. The document discusses concepts related to gravitation including Newton's universal law of gravitation, Kepler's laws of planetary motion, acceleration due to gravity, mass, weight, thrust, pressure, and equations of vertical motion.
2. Key figures discussed include Johannes Kepler, Isaac Newton, and Archimedes. Newton developed the universal law of gravitation and Kepler described three empirical laws of planetary motion.
3. The universal law of gravitation states that the gravitational force between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
Newton's theory of universal gravitation proposes that every object in the universe attracts every other object with a force proportional to the product of their masses and inversely proportional to the square of the distance between them. Newton realized that the moon and falling apples are attracted to Earth by the same force of gravity. He determined gravitational forces exist between all objects and derived the inverse-square law formula to calculate these forces. Examples of applying Newton's theory include calculating the masses of Earth and Sun from their gravitational interactions, and determining satellite speeds and orbital distances using formulas balancing gravitational and centrifugal forces.
1. The document discusses gravity and its role in planetary orbits in the solar system.
2. It explains how Galileo's measurements of gravitational acceleration on Earth helped revolutionize theories of gravity.
3. Isaac Newton then developed his law of universal gravitation, which explained planetary orbits by proposing gravity depends on the inverse square of the distance between objects and is proportional to their masses.
1. The document discusses concepts related to gravitation including Newton's Universal Law of Gravitation, Kepler's Laws of Planetary Motion, gravitational force, and acceleration due to gravity.
2. Key points covered include Newton's inverse square law formula for gravitational force, Kepler's three laws of planetary motion, and definitions of free fall and acceleration due to gravity.
3. The document also discusses properties of gravitational force and provides examples to illustrate concepts like why objects on Earth do not continuously accelerate towards each other due to gravitational attraction.
The document discusses concepts related to gravitation including:
1. Newton's universal law of gravitation which states that the gravitational force between two bodies is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
2. Kepler's laws of planetary motion which describe the motion of planets around the sun, including that planets move in elliptical orbits with the sun at one focus.
3. The acceleration due to gravity on Earth is approximately 9.8 m/s2 and causes objects with mass to have weight, defined as the gravitational force on an object.
The document discusses concepts related to gravitation including Newton's universal law of gravitation, Kepler's laws of planetary motion, acceleration due to gravity, and equations of vertical motion. Some key points covered include:
1) Newton's universal law of gravitation states that the gravitational force between two bodies is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
2) Kepler's laws describe the motion of planets and include that planets move in elliptical orbits with the sun at one focus.
3) Acceleration due to gravity on Earth is approximately 9.8 m/s2 and causes objects to experience weight. Weight depends on both mass and location.
This document discusses Sir Isaac Newton and Johannes Kepler's contributions to the understanding of gravitation. It covers Newton's universal law of gravitation, Kepler's laws of planetary motion, gravitational force, acceleration due to gravity, equations of vertical motion, mass, weight, thrust, pressure, Archimedes' principle, and density. Key points include Newton's inverse square law of gravitation, Kepler's three laws of planetary motion, how gravitational force causes objects to accelerate at 9.8 m/s2 on Earth, and how pressure depends on both force and contact area.
Gravitation is a force that attracts two masses towards each other. Newton's Law of Universal Gravitation states that the gravitational force between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between them. Albert Einstein later developed the theory of gravitation further in his theories of relativity. On Earth, the acceleration due to gravity is approximately 9.8 m/s2, causing objects to fall towards the ground when dropped.
The document discusses concepts related to gravitation including:
1. Key figures who contributed to our understanding of gravitation such as Johannes Kepler and Isaac Newton. Kepler's laws of planetary motion and Newton's universal law of gravitation are summarized.
2. Properties of gravitational force such as it being the weakest force, attractive, and obeying an inverse square law.
3. How the gravitational force between celestial bodies causes tides, and details on lunar tides and their relationship to phases of the moon.
This document provides a detailed overview of universal gravitation and its discovery. It discusses how Kepler summarized astronomical data and formulated his three laws of planetary motion in the early 1600s. Newton then used thought experiments involving cannonballs to deduce that gravity causes objects to fall and that the force of gravity follows an inverse-square law, decreasing with the square of the distance between objects. The document also explains how Cavendish experimentally determined the gravitational constant G.
1) There are four main types of forces - gravitational, electromagnetic, nuclear, and centripetal. Gravitational force acts between any two masses and depends on their masses and the distance between them.
2) Kepler's laws of planetary motion describe the motion of planets in the solar system. Newton's universal law of gravitation states that there is a gravitational attraction between any two masses that is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
3) Gravitational acceleration (g) is the acceleration on an object due to gravity. On Earth, g is approximately 9.8 m/s2. The value of g depends on factors like the
1) Gravity is a natural phenomenon that causes all objects with mass to attract each other. Modern physics describes gravitation through Einstein's general theory of relativity, which views gravity as a distortion of spacetime by massive objects.
2) Isaac Newton formulated the law of universal gravitation, which states that the gravitational force between two objects is directly proportional to their masses and inversely proportional to the square of the distance between them.
3) Newton's theory accounted for the motions of celestial bodies and dominated scientists' views of the physical universe for three centuries, until Einstein's general relativity resolved some discrepancies like Mercury's orbit.
The Civic Welfare Training and Service Module is designed to equip individuals with the knowledge and skills necessary for active participation in community development. Through a comprehensive curriculum, participants engage in theoretical and practical aspects of civic responsibilities, social issues, and community outreach. This module aims to foster a sense of social responsibility and empower participants to contribute meaningfully to the well-being of society through various service initiatives.
The Bambang Elementary School in Pasig City has created a School Action Plan for its Supreme Pupil Government (SPG) for the 2018-2019 school year. The plan outlines activities for each month from May to March focused on cleanliness drives, celebrations, campaigns, and meetings. Key events include Brigada Eskwela in May, a Friendship Day in June, various celebrations and campaigns throughout the year, and the induction of new SPG officers in March. The plan aims to promote student leadership and involvement in bettering the school.
This document discusses RPMS tools and performance indicators for teachers in the Philippines. It explains that there are two RPMS tools for different levels of teachers that assess them on key result areas, objectives, means of verification, and performance indicators. It provides examples of how a Teacher I and Master Teacher I would be assessed and rated using their submitted means of verification for various objectives. Sample scenarios show the teacher's quality and efficiency ratings, average rating, and overall score. The document aims to help teachers and evaluators understand how to use the RPMS tools and what documentation to include for assessment.
Gravitation, free fall, variation in 'g' and keplers law lecture wiseRohan Jain
?
This document contains lecture notes on gravitational force and Newton's law of universal gravitation. It discusses key topics including:
- Gravitational force is a fundamental force that attracts all objects with mass. Newton's law of gravitation describes the force as directly proportional to the product of the masses and inversely proportional to the square of the distance between them.
- Kepler's laws of planetary motion describe how planets move in elliptical orbits with the sun at one focus. Kepler's first law states orbits are ellipses, the second that planets sweep out equal areas in equal times, and the third relates orbital periods to orbital radii.
- The value of the gravitational acceleration g varies depending on location, altitude,
1. The document discusses concepts related to gravitation including Newton's universal law of gravitation, Kepler's laws of planetary motion, acceleration due to gravity, mass, weight, thrust, pressure, and equations of vertical motion.
2. Key figures discussed include Johannes Kepler, Isaac Newton, and Archimedes. Newton developed the universal law of gravitation and Kepler described three empirical laws of planetary motion.
3. The universal law of gravitation states that the gravitational force between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
Newton's theory of universal gravitation proposes that every object in the universe attracts every other object with a force proportional to the product of their masses and inversely proportional to the square of the distance between them. Newton realized that the moon and falling apples are attracted to Earth by the same force of gravity. He determined gravitational forces exist between all objects and derived the inverse-square law formula to calculate these forces. Examples of applying Newton's theory include calculating the masses of Earth and Sun from their gravitational interactions, and determining satellite speeds and orbital distances using formulas balancing gravitational and centrifugal forces.
1. The document discusses gravity and its role in planetary orbits in the solar system.
2. It explains how Galileo's measurements of gravitational acceleration on Earth helped revolutionize theories of gravity.
3. Isaac Newton then developed his law of universal gravitation, which explained planetary orbits by proposing gravity depends on the inverse square of the distance between objects and is proportional to their masses.
1. The document discusses concepts related to gravitation including Newton's Universal Law of Gravitation, Kepler's Laws of Planetary Motion, gravitational force, and acceleration due to gravity.
2. Key points covered include Newton's inverse square law formula for gravitational force, Kepler's three laws of planetary motion, and definitions of free fall and acceleration due to gravity.
3. The document also discusses properties of gravitational force and provides examples to illustrate concepts like why objects on Earth do not continuously accelerate towards each other due to gravitational attraction.
The document discusses concepts related to gravitation including:
1. Newton's universal law of gravitation which states that the gravitational force between two bodies is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
2. Kepler's laws of planetary motion which describe the motion of planets around the sun, including that planets move in elliptical orbits with the sun at one focus.
3. The acceleration due to gravity on Earth is approximately 9.8 m/s2 and causes objects with mass to have weight, defined as the gravitational force on an object.
The document discusses concepts related to gravitation including Newton's universal law of gravitation, Kepler's laws of planetary motion, acceleration due to gravity, and equations of vertical motion. Some key points covered include:
1) Newton's universal law of gravitation states that the gravitational force between two bodies is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
2) Kepler's laws describe the motion of planets and include that planets move in elliptical orbits with the sun at one focus.
3) Acceleration due to gravity on Earth is approximately 9.8 m/s2 and causes objects to experience weight. Weight depends on both mass and location.
This document discusses Sir Isaac Newton and Johannes Kepler's contributions to the understanding of gravitation. It covers Newton's universal law of gravitation, Kepler's laws of planetary motion, gravitational force, acceleration due to gravity, equations of vertical motion, mass, weight, thrust, pressure, Archimedes' principle, and density. Key points include Newton's inverse square law of gravitation, Kepler's three laws of planetary motion, how gravitational force causes objects to accelerate at 9.8 m/s2 on Earth, and how pressure depends on both force and contact area.
Gravitation is a force that attracts two masses towards each other. Newton's Law of Universal Gravitation states that the gravitational force between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between them. Albert Einstein later developed the theory of gravitation further in his theories of relativity. On Earth, the acceleration due to gravity is approximately 9.8 m/s2, causing objects to fall towards the ground when dropped.
The document discusses concepts related to gravitation including:
1. Key figures who contributed to our understanding of gravitation such as Johannes Kepler and Isaac Newton. Kepler's laws of planetary motion and Newton's universal law of gravitation are summarized.
2. Properties of gravitational force such as it being the weakest force, attractive, and obeying an inverse square law.
3. How the gravitational force between celestial bodies causes tides, and details on lunar tides and their relationship to phases of the moon.
This document provides a detailed overview of universal gravitation and its discovery. It discusses how Kepler summarized astronomical data and formulated his three laws of planetary motion in the early 1600s. Newton then used thought experiments involving cannonballs to deduce that gravity causes objects to fall and that the force of gravity follows an inverse-square law, decreasing with the square of the distance between objects. The document also explains how Cavendish experimentally determined the gravitational constant G.
1) There are four main types of forces - gravitational, electromagnetic, nuclear, and centripetal. Gravitational force acts between any two masses and depends on their masses and the distance between them.
2) Kepler's laws of planetary motion describe the motion of planets in the solar system. Newton's universal law of gravitation states that there is a gravitational attraction between any two masses that is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
3) Gravitational acceleration (g) is the acceleration on an object due to gravity. On Earth, g is approximately 9.8 m/s2. The value of g depends on factors like the
1) Gravity is a natural phenomenon that causes all objects with mass to attract each other. Modern physics describes gravitation through Einstein's general theory of relativity, which views gravity as a distortion of spacetime by massive objects.
2) Isaac Newton formulated the law of universal gravitation, which states that the gravitational force between two objects is directly proportional to their masses and inversely proportional to the square of the distance between them.
3) Newton's theory accounted for the motions of celestial bodies and dominated scientists' views of the physical universe for three centuries, until Einstein's general relativity resolved some discrepancies like Mercury's orbit.
- The document discusses Newton's formulation of the universal law of gravitation. It explains that Newton realized that the same gravitational force that causes apples and other objects on Earth to fall also causes the moon to orbit Earth and planets to orbit the Sun.
- The universal law of gravitation states that every object in the universe attracts every other object with a force proportional to the product of their masses and inversely proportional to the square of the distance between them.
- The document provides an example calculation of the gravitational force between Earth and the moon using the universal law of gravitation.
The document discusses Isaac Newton's formulation of the universal law of gravitation. It explains that Newton realized that the same gravitational force that causes apples and other objects on Earth to fall also causes the moon to orbit Earth and planets to orbit the Sun. The universal law of gravitation states that every object in the universe attracts every other object with a force proportional to the product of their masses and inversely proportional to the square of the distance between them. The document also provides background on Newton and outlines some important implications and applications of the universal law of gravitation.
1. The document discusses key concepts of gravitation including Newton's universal law of gravitation, Kepler's laws of planetary motion, gravitational force, acceleration due to gravity, escape velocity, and free fall.
2. It explains that gravitational force is responsible for holding the atmosphere above the earth and for the motion of objects.
3. Newton's universal law of gravitation states that the gravitational force between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.
Gravity is a fundamental force that causes objects with mass to accelerate towards each other. Kepler determined that planetary orbits are elliptical rather than circular, and that planets move faster when closer to the sun. Newton realized that the force causing apples and the moon to move was gravity. His law of universal gravitation stated that the gravitational force between objects is directly proportional to their masses and inversely proportional to the square of the distance between them. Gravity creates gravitational fields around massive objects that other objects interact with. Tides are caused by differences in the moon's gravitational pull on the near and far sides of Earth.
芙坪茶氏Y創_Data-Centric AI in The Age of Large Language Models鰻粥京晦粥皆幄塀氏芙
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このY創では、LLMの撹孔にはデ`タの|と謹來が音辛之であることをh苧しています。愔瓦離皀妊觚追屯佩弔離▲廛踪`チにし、デ`タ嶄伉のAI_kを戻宛し、より紳糞弔罵乎來の互いLLMのBに鬚韻疹潴綉弔癖峽┐鮟B初しています。デ`タの恷m晒や試喘圭隈、販あるAI_kの嶷勣來についても乾れられており、LLMのパフォ`マンス鯢呂墨鬚韻塵造燭片泣を戻工する坪否です。
This paper explains that the success of LLMs depends heavily on the quality and diversity of data. Instead of focusing solely on model improvements, it proposes a data-centric approach to AI development, introducing concrete methods for building more efficient and transparent LLMs. It also discusses data optimization, utilization strategies, and the importance of responsible AI development, offering a fresh perspective on enhancing LLM performance.
Better Builder Magazine brings together premium product manufactures and leading builders to create better differentiated homes and buildings that use less energy, save water and reduce our impact on the environment. The magazine is published four times a year.
David Boutry - A Senior Software EngineerDavid Boutry
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David Boutry is a Senior Software Engineer based in New York with over eight years of experience in AWS, microservices, Python, and JavaScript. He led a team that enhanced data processing efficiency by 40% and previously optimized e-commerce applications in Seattle, boosting sales by 25%. Passionate about mentorship and community engagement, David organizes coding workshops and develops software solutions for nonprofits.
Amazon Web Services (AWS) is a popular cloud platform praised for its scalability, flexibility, and extensive range of services, making it a good choice for businesses of all sizes.
Battery charging technology for electric vehicle.pptxVirajPasare
?
Types of battery charging, Normal charging, Opportunity charging, Fast charging, Constant current and constant voltage Charging, Multistage charging (MSC), Pulse Charging, Trickle Charging (TC).
Chapter 2.pdf Smith Chart and Impedance Matchingdathoang3243
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gravity report
1. REPORT ON GRAVITY
HISTORY OF GRAVITY:
The understanding and exploration of gravity have a long history that dates back to ancient
civilizations. Here is a brief overview of the historical developments in our understanding of
gravity.
SCIENTIFIC REVOLUTION AND NEWTON:
? The modern understanding of gravity began to take
shape during the scientific revolution in the 16th and
17th centuries. Galileo Galilei conducted experiments on falling objects and
demonstrated that all objects, regardless of their mass, fall towards the Earth at the
same rate (discounting the effects of air resistance).
? Sir Isaac Newton, in the late 17th century, developed his laws of motion and the law
of universal gravitation. Newton's law of universal gravitation stated that every
particle in the universe attracts every other particle with a
force that is directly proportional to their masses and
inversely proportional to the square of the distance
between them.
? Newton's laws of motion and his law of universal
gravitation provided a comprehensive framework for understanding and calculating
the motion of objects under the influence of gravity. This laid the foundation for
classical mechanics and revolutionized the field of physics.
REFINEMENTS AND ADVANCEMENTS:
? In the 19th century, advancements in astronomy and celestial mechanics led to more
precise measurements of planetary motion. Johann Kepler's laws of planetary motion,
combined with Newton's laws of motion and gravitation, provided a deeper
understanding of the dynamics of celestial bodies.
2. ? Albert Einstein's theory of general relativity,
published in 1915, revolutionized our understanding
of gravity. General relativity describes gravity as
the curvature of space-time caused by mass and
energy. It provided a new framework for
understanding gravity's behavior in extreme
conditions, such as near black holes or during the
expansion of the universe.
? Since Einstein, the study of gravity has continued to evolve through theoretical
advancements and experimental observations. Modern theories, such as quantum
gravity, attempt to reconcile general relativity with quantum mechanics to provide a
unified theory of gravity at the smallest scales.
The understanding of gravity has evolved significantly throughout history, from ancient
philosophical speculations to the precise mathematical descriptions of Newton and the
revolutionary insights of Einstein. The ongoing research and exploration in the field continue
to deepen our understanding of gravity's fundamental nature and its role in the workings of
the universe.
GRAVITY:
Gravity is a fundamental force of nature that governs the attraction between objects with
mass or energy. It is responsible for holding planets in orbit around stars, moons in orbit
around planets, and objects on Earth's surface.
The standard value for "small g" on the surface of the Earth is
approximately 9.8 meters per second squared (m/s?). This
means that when an object is in free fall near the Earth's
surface, it accelerates at a rate of approximately 9.8 m/s?
towards the center of the Earth due to the force of gravity.
It's important to note that "small g" is an acceleration and
should not be confused with "big G," which represents the
3. gravitational constant in the law of universal gravitation (as mentioned in the previous
response).
VALUE OF GRAVITY:
The value of gravity refers to the acceleration due to gravity, which is a constant value that
determines the strength of the gravitational force between two objects. On Earth, the average
value of the acceleration due to gravity is approximately 9.8
meters per second squared (m/s?).
This means that when an object near the surface of the Earth
is in free fall, it accelerates at a rate of 9.8 m/s? towards the
center of the Earth. This acceleration is often represented by
the symbol "g" and is commonly rounded to 9.8 m/s? for
simplicity in calculations.
DEPENDING:
It's important to note that the value of gravity can vary depending on the location and altitude
on Earth's surface. For example, at higher altitudes, the value of gravity is slightly lower due
to the increased distance from the center of the Earth. Additionally, gravity can vary on
different celestial bodies based on their mass and size.
In scientific calculations and formulas involving gravity, the precise value of the acceleration
due to gravity (g) is used, which can be measured more accurately through experimentation
and calculations.
RELATION OF GRAVITY WITH WEIGHT:
Gravity and weight are closely related concepts. Weight is the force exerted on an object due
to gravity. It is the measure of the gravitational force acting on an object's mass.
The weight of an object can be calculated using the formula:
Weight = mass * acceleration due to gravity
4. In this formula, the mass of the object is multiplied by the acceleration due to gravity to
determine the force of gravity acting on the object, which is its
weight. The acceleration due to gravity is represented by the
symbol "g" and has an average value of approximately 9.8 m/s?
on Earth's surface.
EXAMPLE:
So, if you have the mass of an object, you can determine its weight by multiplying the mass
by the acceleration due to gravity. For example, if an object has a mass of 10 kilograms on
Earth, its weight would be:
Weight = 10 kg * 9.8 m/s? = 98 Newton
Therefore, the weight of the object would be 98 newton.
It's important to note that weight is a force and is measured in newton (N), whereas mass is a
measure of the amount of matter in an object and is typically measured in kilograms (kg).
Weight can vary depending on the strength of gravity at a particular location or on different
celestial bodies, whereas mass remains constant regardless of the gravitational field.
LAW OF GRAVITATIONAL FORCE:
According to Isaac Newton's law of universal gravitation, the force of gravity between two
objects is directly proportional to the product of their masses and inversely proportional to
the square of the distance between them. Mathematically, it can be expressed as:
Where:
- F is the force of gravity between the two objects.
5. - G is the gravitational constant (approximately 6.67430 〜 10^-11 N (m/kg) ^2).
- m1 and m2 are the masses of the two objects.
- R is the distance between the centers of the two objects.
Gravity is responsible for keeping celestial bodies in their respective orbits and also
determines the weight of objects on Earth's surface. It is a fundamental force that plays a
crucial role in shaping the structure and behavior of the universe.
GRAVITATIONAL FIELD STRENGTH
The gravitational field strength, denoted by "g" or "g-field," represents the magnitude of the
gravitational field at a specific point. It is defined as the force experienced per unit mass by
an object placed at that point. The gravitational field
strength is given by:
g = F / m
Where:
? g is the gravitational field strength.
? F is the gravitational force experienced by the mass.
? m is the mass of the object experiencing the gravitational field.
The direction of the gravitational field is always towards the center of the mass creating the
field. In other words, it points in the direction of the gravitational force that an object would
experience if placed at that point.
In summary, gravitational force describes the attraction between masses, while the
gravitational field represents the influence of gravity in space. The gravitational field
determines the force experienced by objects with mass within that field.
6. GRAVITATIONAL POTENTIAL:
The concept of gravitational potential is closely related to the concept of gravitational field
strength. The field strength (g) at a point is the rate of change of gravitational potential with
distance:
This relationship helps determine the gravitational force experienced by an object at a given
point, as the force is proportional to the field strength.
In summary, gravitational potential is a measure of the potential energy per unit mass
associated with an object in a gravitational field. It quantifies the work done to bring an
object from infinity to a specific location and is an essential concept in understanding the
behavior of objects in the presence of gravity.
EINSTEIN¨S VIEW ON GRAVITY
Albert Einstein revolutionized our understanding of gravity with his theory of general
relativity, which he proposed in 1915.
Einstein's view of gravity significantly differed
from the classical Newtonian understanding.
According to Einstein's general theory of
relativity, gravity is not simply a force acting at a distance, as described by Newton's law of
universal gravitation. Instead, Einstein proposed that gravity arises due to the curvature of
space time caused by the presence of mass and energy.
7. Einstein's theory states that massive objects, such as planets or stars, warp the fabric of space
time around them. This warping of space time creates what we perceive as gravity.
Essentially, objects with mass and energy tell space time how to curve, and the curved space
time tells objects how to move.
GENERAL THEORY OF RELATIVITY
Einstein's general theory of relativity, often referred
to as simply general relativity, is a theory of gravity
proposed by Albert Einstein in 1915. It provides a
new understanding of gravity that goes beyond
Newtonian physics and has been incredibly
successful in explaining various gravitational phenomena and cosmological observations.
KEY PRINCIPLES OF GENERAL RELATIVITY:
Equivalence Principle: The equivalence principle states that there is no difference between
the effects of gravity and the effects of acceleration. In other words, the force of gravity
experienced by an object is equivalent to the force experienced when the object is accelerated
in the absence of gravity.
1. Curvature of Space-time: General relativity introduces the concept that mass and
energy curve or deform the fabric of space time. The presence of mass and energy
causes space-time to be curved, and objects moving within this curved space time
follow curved paths.
2. Geodesics and Gravity: In general relativity, the motion of
objects is determined by following the geodesics (the shortest
paths) in curved space time. Objects move along the most
efficient paths through the curved space time, which results in
the appearance of gravitational attraction.
8. 3. Gravitational Time Dilation: General relativity predicts that time passes at different
rates in regions with different gravitational fields. Clocks in stronger gravitational
fields appear to run slower compared to clocks in weaker gravitational fields.
4. Bending of Light: According to general relativity, the presence of mass and energy
can cause the curvature of space-time, leading to the bending of light as it passes
through the gravitational field. This effect has been confirmed by experiments and
observations, such as the bending of starlight near the Sun during a solar eclipse.
APPLICATIONS AND CONFIRMATIONS:
General relativity has provided successful
explanations for a range of phenomena and has
been confirmed by numerous experimental tests and astronomical observations, including:
? The precession of Mercury's orbit: General relativity correctly accounts for the
observed discrepancy in the orbit of Mercury compared to predictions based on
Newtonian physics.
? Gravitational lensing: The bending of light by massive objects, such as galaxies or
clusters of galaxies, has been observed and confirmed in line with the predictions of
general relativity.
? Time dilation and gravitational redshift: Precise experiments have confirmed the
effects of time dilation and gravitational redshift, demonstrating the impact of gravity
on the flow of time and the frequency of light.
? Gravitational waves: In 2015, the first direct detection of gravitational waves, ripples
in space time caused by the motion of massive objects, was made, providing direct
evidence for the existence of these waves as predicted by general relativity.
Overall, Einstein's general relativity revolutionized our understanding of gravity and remains
one of the most successful and widely accepted physical theories to date. It has far-reaching
implications for our understanding of the universe, from the behavior of black holes to the
expansion of the universe on a cosmological scale.
9. GRAVITY AND LIGHT:
Gravity and light are interconnected in several ways according to Einstein's theory
of general relativity.
1. Gravitational Lensing: Gravity can bend the path of
light as it travels through a gravitational field. Massive
objects, such as stars or galaxies, can act as lenses, causing the light
from more distant objects to bend as it passes by. This phenomenon is known as
gravitational lensing. It has been observed and confirmed, and it provides a way to
study distant objects and test the predictions of general relativity.
2. Time Dilation and Frequency Shift: According to
general relativity, the flow of time is affected by
gravitational fields. In regions of stronger gravity, time
passes more slowly compared to regions of weaker
gravity. This means that light traveling through a gravitational field experiences a
change in its frequency. This effect is known as gravitational redshift or blue shift,
depending on whether the light is moving away from or towards the gravitational
source, respectively.
3. Black Holes: Black holes are extremely massive objects that have such strong
gravitational fields that nothing, including light, can
escape their gravitational pull within a certain boundary
called the event horizon. The concept of black holes
arises from the predictions of general relativity. Light
that approaches the event horizon of a black hole will be
pulled in and cannot escape, leading to the formation of
a dark region.
4. Gravitational Waves: Gravitational waves are ripples
in space-time caused by the acceleration of massive objects. They travel at the speed
of light and carry energy away from the source. The detection of gravitational waves
10. provides direct evidence of the existence of these waves and confirms Einstein's
predictions. Gravitational waves have been detected from the mergers of black holes
and neutron stars, demonstrating the coupling between gravity and the propagation of
light.
In summary, gravity can bend the path of light, affect its frequency and energy, create black
holes where light cannot escape, and produce gravitational waves that travel at the speed of
light. These phenomena highlight the deep connection between gravity and light as described
by Einstein's theory of general relativity.
RAINBOW GRAVITY THEORY
Rainbow gravity theory is a speculative and alternative theory of gravity that proposes
modifications to Einstein's general theory of relativity. It suggests that the effects of gravity
on space-time may depend on the energy of particles or photons traveling through it, leading
to a modification of the usual gravitational equations.
The term "rainbow" in rainbow gravity theory refers to the concept that different particles
with varying energies experience different gravitational effects, much like how different
colors of light refract at different angles to form a rainbow.
The theory was first proposed by
theoretical physicist Giovanni
Amelino-Camelia in 2013 as a
possible approach to address
certain issues in the framework of
quantum gravity. Rainbow
gravity theory incorporates
elements from both quantum mechanics and general relativity, aiming to provide a more
comprehensive understanding of gravity at both small and large scales.
11. KEY IDEAS IN RAINBOW GRAVITY THEORY
The energy-dependent modification of space-time curvature could potentially resolve some
of the challenges faced by other theories, such as the incompatibility between quantum
mechanics and general relativity at very high energy scales or the singularity problem at the
center of black holes.
However, it is important to note that rainbow gravity theory is still a highly speculative
concept, and it has not yet gained widespread acceptance or experimental confirmation. It
remains an area of active research and theoretical exploration within the field of quantum
gravity and the quest for a unified theory of physics.
Further research and experimental evidence will be needed to determine the validity and
implications of rainbow gravity theory and its compatibility with existing observations and
fundamental principles of physics.
GRAVITY BETWEEN SPHERICAL BODIES
Newton's law of gravitation describes the gravitational force between any two point masses.
However, for extended spherical objects like the Earth, the Moon, and other planets, the law
holds with an assumption that masses of spherical objects are concentrated at their respective
centers.
This assumption can be
proved easily by showing that the expression for gravitational potential energy between a
hollow sphere of mass (M) and a point mass (m) is the same as it would be for a pair of
extended spherical solid objects.
12. Consider a tiny ring of width Rd? and mass dM on the surface of a spherical hollow sphere at
a distance s from the point mass as shown in Figure 1(a).
The gravitational potential energy between the ring and the point mass (m) is expressed as:
The ratio of the ring's mass to the entire shell's mass is equal to the ratio of the ring's area to
the shell's area. Therefore, on simplification, the ring's mass can be expressed as:
Now, the square of distance (s) can be expressed as the sum of squares of the triangle's other
two sides, as seen in Figure 1(b).
Simplifying further and taking differentials on either side,
Considering the entire shell, s can vary between r ? R and r + R, as seen in Figure 1(c).
Therefore, substituting dM and s in the potential energy equation and integrating within the
limits of r ? R to r + R, the relation obtained is the potential energy between point
masses m and M at a distance r.
Therefore, the assumption is proven.
Since force is a derivative of potential energy, the assumption holds for gravitational forces
between two spherically solid objects like the Earth and the Moon. Therefore, Newton's law
of gravitation can be used to determine the gravitational force between the Earth and the
Moon, and the Earth and the Sun.
13. QUANTUM GRAVITY (QG):
Quantum gravity (QG) is a field of theoretical physics that seeks to describe gravity
according to the principles of quantum mechanics. It deals
with environments in which neither gravitational nor
quantum effects can be ignored such as in the vicinity of
black holes, such as neutron stars.
Quantum mechanics describes the behavior of matter and
energy on very small scales, such as atoms and subatomic particles, while general relativity
describes the force of gravity and the behavior of matter and energy on large scales, such as
stars, galaxies, and the universe as a whole.
RELATION OF CLASSICAL PHYSICS:
In classical physics, gravity is described as a continuous force that can be described by
Einstein's field equations in general relativity. However, when attempting to incorporate the
principles of quantum mechanics, several challenges arise. One of the main issues is that the
equations of general relativity do not account for the behavior of gravity at extremely small
distances or at the singularities that arise in black holes.
Quantum gravity seeks to develop a theory that encompasses both quantum mechanics and
general relativity, providing a consistent description of the gravitational force at all scales. It
aims to explain how gravity arises from the quantum behavior of fundamental particles and
fields, and how the curvature of space-time, described by general relativity, can be
understood in a quantum framework.
SPACE-TIME BACKGROUND DEPENDENCE:
Background independence is considered desirable because it allows for a more fundamental
and unified treatment of gravity and other interactions. It enables a description of the
gravitational field itself as a quantum entity and allows for a consistent quantum description
of the early universe and black hole singularities, where the classical notion of spacetime
breaks down.
14. Developing a background-independent theory of quantum gravity is an active area of
research, and various approaches and formalisms are being explored to overcome the
challenges posed by background dependence and achieve a deeper understanding of the
fundamental nature of space time and gravity.
PROBLEM OF TIME:
A conceptual difficulty in combining quantum mechanics with general relativity arises from
the contrasting role of time within these two frameworks. In quantum theories time acts as an
independent background through which states evolve, with the Hamiltonian operator acting
as the generator of infinitesimal translations of quantum states through time. In contrast,
general relativity treats time as a dynamical variable which relates directly with matter and
moreover requires the Hamiltonian constraint to vanish. Because this variability of time has
been observed macroscopically, it removes any possibility of employing a fixed notion of
time, similar to the conception of time in quantum theory, at the macroscopic level.
LOOP QUANTUM GRAVITY:
Loop quantum gravity (LQG) is a theoretical framework and approach to quantum gravity
that aims to quantize the geometry of space time.
In loop quantum gravity, space time is discretized into a network of elementary units called
loops or spin networks. These loops are based on the mathematical framework of spin
networks from the theory of quantum mechanics. The theory incorporates principles from
both general relativity and quantum mechanics to describe the quantum behavior of these
loops.
WHEELER-DEWITT EQUATION:
The dynamics of loop quantum gravity are described by the Hamiltonian constraint equation,
known as the Wheeler-DeWitt equation in the canonical quantization of general relativity.
However, in loop quantum gravity, the Wheeler-DeWitt equation is modified and
reformulated to incorporate the discrete nature of space time.
15. The Wheeler-DeWitt equation can be written as:
Here, ? is the Wheeler-DeWitt operator, which represents the Hamiltonian constraint. It is an
operator that acts on a wave function of the universe, denoted by Ψ. The wave function Ψ
describes the quantum state of the entire universe or the space-time geometry itself.
The Wheeler-DeWitt equation essentially states that the total wave function of the universe
must satisfy this constraint equation. It implies that the Hamiltonian of the system, which
generates time evolution in classical physics, vanishes when acting on the wave function.
STRING THEORY:
String theory is a theoretical framework that combines quantum mechanics and general
relativity to describe the fundamental building blocks of the universe as tiny, vibrating
strings instead of point-like particles
KEY FEATURES OF STRING THEORY:
1. Extended Objects: In contrast to point particles, which have no internal structure,
string theory introduces one-dimensional strings. These strings can vibrate and
undergo different modes of oscillation, giving rise to different particle properties such
as mass, charge, and spin. The vibrational patterns of the strings determine the various
types of particles observed in nature.
2. Extra Dimensions: String theory also requires the existence of additional spatial
dimensions beyond the familiar three dimensions of space (length, width, and height)
and the dimension of time. These extra dimensions are typically curled up" at very
16. small scales, making them effectively unobservable at everyday energy scales. The
inclusion of extra dimensions helps resolve certain mathematical and conceptual
issues that arise in attempts to unify gravity with the other fundamental forces.
3. Consistency and Symmetry: String theory incorporates principles of quantum
mechanics, such as wave-particle duality and uncertainty, as well as the principles of
general relativity. It maintains consistency through a set of mathematical rules
governing the interactions and behavior of the strings. Symmetry plays a crucial role
in string theory, with various symmetries offering insights into the relationships
between different particles and forces.
4. String Theory Landscape: String theory predicts a vast landscape of possible solutions
or "vacua," each corresponding to a different set of physical properties, including
particle masses and coupling constants. This concept of a landscape provides a
potential explanation for the diverse phenomena observed in our universe.
It is important to note that string theory is still an area of active research, and many aspects
of the theory are yet to be fully understood. The theory exists in various formulations and
versions, including Type I, Type IIA, Type IIB, heterotic, and M-theory, which are different
limits or dual descriptions of a more fundamental theory.
CONCEPTS IN STRING THEORY:
1. Nambu-Goto Action: The Nambu-Goto action describes the dynamics of a string in
terms of its worldsheet, a two-dimensional surface swept out by the string as it moves
through spacetime. The action is proportional to the area of the worldsheet and is
given by:
S = -T〈d?σ 〔(-h)
Here, T is the string tension, d?σ represents the worldsheet area element, and h is the
determinant of the worldsheet metric.
2. String Mode Expansion: The equations of motion in string theory involve the
expansion of the string coordinates and fields into different modes of vibration. These
17. modes represent the various vibrational states of the string, corresponding to different
particles and interactions. The specific equations for the mode expansion depend on
the type of string theory being considered (e.g., open strings or closed strings) and the
specific background conditions.
It's important to note that the full equations of string theory are highly complex and
involve sophisticated mathematical techniques, such as conformal field theory, super
symmetry, and extra dimensions. The equations mentioned above provide a glimpse into
the mathematical framework of string theory, but a complete and unified formulation of
the theory is still an active area of research.