Physics, asked by architjain2007, 4 months ago

reply fast with explanation
Before the theory of relativity, scientists called the reference point for all motion as,
a. Focal Point
b. The Earth
c. Ether
d. The Sun
fast plz give explanation​


kanak8398: hii

Answers

Answered by 21911
0

Answer:

Einstein’s theory of relativity has a formidable reputation as

being incredibly complicated and impossible to understand.

It’s not! The principle of relativity itself, the single, simple

idea upon which Einstein’s theory is based, has been around

since the time of Galileo. As we shall see, when it is applied

to objects that are moving extremely fast, the consequences

seem strange to us because they are outside our everyday ex-

perience; but the results make sense and are all self-consistent

when we think about them carefully. We can summarize the

major corrections that we need to make to Newton’s equations

of motion as follows: Firstly, when an object is in motion, its

momentum p is larger than expected, its length l shrinks in

the direction of motion, and time t slows down, in each case

by a factor

γ = 1

1 − v2/c2

, (2.1)

where v is the velocity of the object and c is the speed of light:

c = 299792458m/s(exactly, bydefinition)

= 186, 282miles/second

= 30cm/ns, inunitswecangrasp.This seems confusing at first because we are used to assuming,

for example, that the length l of any object should be constant.

For everyday purposes, the correction is tiny — consider the

International Space Station, moving at 8 km/s in orbit; its

length is about 1 part per billion less than if it were at rest,

and time on board moves more slowly by the same factor. But

for many particles moving near the speed of light, the fact that

time slows down (and hence lifetimes are longer) with velocity

by the factor (2.1) has been well verified. The same applies to

the increasing momentum – which demonstrates immediately

the well-known principle that one can never push an object

hard enough to accelerate it to the speed of light, since, as it

goes faster and faster, you have to push harder and harder to

obtain a given increase in velocity. Loosely speaking, it acts

as though the mass increases with velocity.

Secondly, as we shall discover about halfway through the

course, there emerges naturally what may well be the most

famous equation in the world:

E = mc2

.These formulae were not found experimentally, but theoret-

ically, as we shall see.

Einstein’s 1905 relativity paper, “On the Electrodynamics

of Moving Bodies”, was one of three he published that year,

at age 26, during his spare time; he was at the time working

as a patent clerk in Zurich. Another was a paper explaining

Brownian motion in terms of kinetic theory (at a time when

some people still doubted the existence of atoms), and the

third proposed the existence of photons, thus laying the foundations for quantum theory and earning him the Nobel prize

(relativity being too controversial then).

Einstein wrote two theories of relativity; the 1905 work is

known as “special relativity” because it deals only with the

special case of uniform (i.e. non-accelerating) motion. In

1915 he published his “general theory of relativity”, dealing

with gravity and acceleration. Strange things happen in accel-

erating frames; objects appear to start moving without any-

thing pushing them... During this course we shall only deal

with special relativity.

2.1 The Principle of Relativity

As we use our telescopes to look ever farther out into the

universe, some relevant questions present themselves:

• Is space homogeneous? I.e., is it the same everywhere —

are the laws of physics the same in distant galaxies as they

are here on Earth?

• Is it isotropic — is it the same in all directions, or is there

some defining “axis” or direction that is preferred in some

way? Is, for example, the speed of light the same in all

directions?

• Are the laws of physics constant in time?

• And finally, are the laws of physics independent of uniform

relative motion?

By looking at light from the most distant visible galaxies,

more than 10 billion light years away, we can recognise the

Answered by kaptansinghsinha517
0

Explanation:

option A

A noun is a word that names something, such as a person, place, thing, or idea. In a sentence, nouns can play the role of subject, direct object, indirect object, subject complement, object complement, appositive, or adjective.A noun is a word that names something, such as a person, place, thing, or idea. In a sentence, nouns can play the role of subject, direct object, indirect object, subject complement, object complement, appositive, or adjective.A noun is a word that names something, such as a person, place, thing, or idea. In a sentence, nouns can play the role of subject, direct object, indirect object, subject complement, object complement, appositive, or adjective.

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