peepal mobile charger screen

Its very Strange But True Very True.

Now, you do not require any mobile charger… to charge your mobiles. Only there is need to use green leaf of peepal tree and after some time your mobile will get charged.

No soon the people came to learn this development, they tested it and found encouraging results. If your mobile has been discharged and you are inside a jungle then you need not to use any charger. You Should pluck two peepal leaves and your work would be done.
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Homi Bhaba

Homi Jehangir Bhabha-The Father of Indian Nuclear Research Prog

Bhabha was born into a wealthy and prominent Parsi family, through which he was related to Dinshaw Maneckji Petit, Muhammad Ali Jinnah and Dorab Tata. He received his early education at Bombay’s Cathedral Grammar School and entered Elphinstone College at age 15 after passing his Senior Cambridge Examination with Honors. He then attended the Royal Institute of Science until 1927 before joining Caius College of Cambridge University. This was due to the insistence of his father and his uncle Dorab Tata, who planned for Bhabha to obtain an engineering degree from Cambridge and then return to India, where he would join the Tata Iron and Steel Company in Jamshedpur.

Return to India : In September 1939, Bhabha was in India for a brief holiday when World War II broke out, and he decided not to return to England for the time being. He accepted an offer to serve as the Reader in the Physics Department of the Indian Institute of Science, then headed by renowned physicist C. V. Raman. He received a special research grant from the Sir Dorab Tata Trust, which he used to establish the Cosmic Ray Research Unit at the institute. Bhabha selected a few students, including Harish-Chandra, to work with him. Later, on 20 March 1941, he was elected a Fellow of the Royal Society . With the help of J. R. D. Tata, he played an instrumental role in the establishment of the Tata Institute of Fundamental Research in Bombay.

Death and legacy : He died when Air India Flight 101 crashed near Mont Blanc on January 24, 1966. Many possible theories have been advanced for the aircrash, including a conspiracy theory in which CIA is involved in order to paralyze Indian nuclear weapon programme. After his death, the Atomic Energy Establishment at Trombay was renamed as the Bhabha Atomic Research Centre in his honour.

In addition to being an able scientist and administrator, Bhabha was also a painter and a classical music and opera enthusiast, besides being an amateur botanist. He is one of the most prominent scientists that India has ever had. Bhabha also encouraged research in electronics, space science, radio astronomy and microbiology. The famed radio telescope at Ooty, India was his initiative, and it became a reality in 1970. The Homi Bhabha Fellowship Council has been giving the Homi Bhabha Fellowships since 1967 Other noted institutions in his name are the Homi Bhabha National Institute, an Indian deemed university and the Homi Bhabha Centre for Science Education, Mumbai, India.

 

Proceed only after investigating, and even then cautiously.
As for keeping the cabinet of your predecessor, there are two approaches.
The first is to start totally anew and dismiss them all. This is recommended only if
you are in possession of enough information about the members, the entity you are
starting to head, and you have an idea that in a relatively short time you will choose
respected new confidants and a new cabinet. Although many new chiefs may find
this approach attractive, it has disadvantages:
1. You are creating enemies unnecessarily.
2. Some dismissed members could be very helpful as they have specific knowledge,
which may be invaluable.
3. Why hurry?

Continue reading “Relations with Senior Staff You Have Inherited” »

 

Should you be so lucky to have choices, select the one that offers the best future
opportunities.
In the economic situation of todays world, to have the luxury of selecting
between two or more attractive job offers in either academia or business is a rare
exception, and if you are in that situation, savor it and choose wisely.
Many universities have frozen new hiring because of curtailments of funding
(from state, city, or church), budget reductions, or endowment losses. Only if you
possess skills that fit with a badly needed requirement will you usually be offered
a position in more than one university.
Should that happen, the choice is usually not too difficult.

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A fundamental problem with the k = 0 universe is that it is unprovable. In fact, assuming
a global FLRW metric, one would require an infinitely precise measurement of
0 = 1 (or equivalent quantity) to demonstrate the flatness of space: any uncertainty
around the (true) critical value can accommodate an infinity of solutions with positive
or negative curvatures. Every physicist knows that no experiment, however precise,
can give results without a finite error bar.
There are deeper uncertainties built in by nature itself that make a spatially flat
universe unprovable. Generally, these are related to limitations in the observability
of the universe by us. A remarkable example applies to CMB data. Even supposing
(unrealistically!) an infinite precision in the measurements of the CMB fluctuations,
the power spectrum would still be limited in accuracy by a cosmic variance because
of the finite statistics of CMB samples that we can observe from a single location in the
universe. This ineliminable uncertainty becomes more important when we probe large
angular scales (??2/(2 + 1)), where only a few independent sky regions (2 + 1)
may be compared to each other to yield the power spectrum coefficients. Current
data at low s are already limited by cosmic variance . To overcome
this limitation, it would be necessary to gather observations of the CMB from several
observers distributed at cosmological distances from each other a possibility that
appears unthinkable. It is possible, therefore, that the answer to our big question on the
finiteness or infinity of the universe is hidden forever inside this kind of fundamental
cosmic uncertainty.
In principle, this limitation might be partly overcome with extremely precise measurements
of the Sunyaev-Zeldovich (SZ) effect18 on large samples of clusters of
galaxies at high redshift (Kamionkowski and Loeb 1997). The basic idea is that SZ
polarized scattering on distant clusters is sensitive to the CMB field as seen by the
cluster; therefore, in principle it can give information on the properties of the surface

” The Sunyaev-Zeldovich effect is inverse Compton scattering of CMB photons off hot electrons in the gas of
clusters of galaxies. Scattered photons are boosted in energy and their spectrum is distorted so that, in the
solid angle subtended by a cluster, we observe a decrease of the CMB temperature at low frequencies and an
increment at high frequencies (for a review see, e.g., Rephaeli 1995).of last scatter as seen by a source at cosmological distance from us. The polarization

Continue reading “The Impossible Proof” »

 

The Quest for Extraterrestrial Intelligence
By Carl Sagan

The Quest for Extraterrestrial Intelligence
By Carl Sagan
Through all of our history we have pondered the stars and mused whether mankind is unique
or if, somewhere else out there in the dark of night sky, there are other beings who
contemplate and wonder as we do – fellow thinkers in the cosmos. Such beings might view
themselves and the universe differently. Somewhere else there might exist exotic biologies,
technologies and societies. What a splendid perspective contact with a profoundly different
civilization might provide! In a cosmic setting vast and old beyond ordinary human
understanding we are a little lonely, and we ponder the ultimate significance, if any, of our tiny
but exquisite blue planet, the Earth. The Search for Extra-Terrestrial Intelligence (SETI) is the
search for a generally acceptable cosmic context for the human species. In the deepest sense
the search for extraterrestrial intelligence is a search for ourselves.
Until recently there could be no such search. No matter how deep the concern or how
dedicated the effort, human beings could not scratch the surface of the problem. But in the
last few years – in one millionth of the lifetime of our species on this planet – we have
achieved an extraordinary technological capability which enables us to seek out unimaginably
distant civilizations, even if they are no more advanced than we. That capability is called radio
astronomy and involves single radio telescopes, collections or arrays of radio telescopes,
sensitive radio detectors, advanced computers for processing received data, and the
imagination and skill of dedicated scientists. Radio astronomy has, in the last decade, opened
a new window on the physical universe. It may also, if we are wise enough to make the effort,
cast a brilliant light on the biological universe.
Some scientists working on the question of extraterrestrial intelligence, myself among them,
have attempted to estimate the number of advanced technical civilizations in the Milky Way
galaxy – that is, societies capable of radio astronomy. Such estimates are little better than
guesses. They require assigning numerical values to quantities such as the numbers and ages
of stars, which we know well; the abundance of planetary systems and the likelihood of the
origin of life within them, which we know less well; and the probability of the evolution of
intelligent life and the lifetime of technical civilizations, about which we know very little
indeed. When we do the arithmetic, the number that my colleagues and I come up with is
around a million technical civilizations in our Galaxy alone. That is a breathtakingly large
number, and it is exhilarating to imagine the diversity, lifestyles and commerce of those million
worlds. But there may be as many as 250 billion stars in the Milky Way Galaxy. Even with a
million civilizations, less than one star in 250,000 would have a planet inhabited by an
advanced civilization. Since we have little idea which stars are likely candidates, we will have to
examine a huge number of them.
Thus the quest for extraterrestrial intelligence may require a significant effort.
Continue reading “The Quest for Extraterrestrial Intelligence By Carl Sagan” »

 

Can We Know the Universe? Reflections on a Grain of Salt
by Carl Sagan


The following excerpt was published in Broca’s Brain (1979)
“Nothing is rich but the inexhaustible wealth of nature. She shows us only surfaces, but
she is a million fathoms deep.” Ralph Waldo Emerson
Science is a way of thinking much more than it is a body of knowledge. Its goal is to find out
how the world works, to seek what regularities there may be, to penetrate the connections of
thingsfrom subnuclear particles, which may be the constituents of all matter, to living
organisms, the human social community, and thence to the cosmos as a whole. Our intuition is
by no means an infallible guide. Our perceptions may be distorted by training and prejudice
or merely because of the limitations of our sense organs, which, of course, perceive directly
but a small fraction of the phenomena of the world. Even so straightforward a question as
whether in the absence of friction a pound of lead falls faster than a gram of fluff was
answered incorrectly by Aristotle and almost everyone else before the time of Galileo. Science
is based on experiment, on a willingness to challenge old dogma, on an openness to see the
universe as it really is. Accordingly, science sometimes requires courageat the very least the
courage to question the conventional wisdom.
Beyond this the main trick of science is to really think of something: the shape of clouds and
their occasional sharp bottom edges at the same altitude everywhere in the sky; the formation
of the dewdrop on a leaf; the origin of a name or a wordShakespeare, say, or
“philanthropic”; the reason for human social customsthe incest taboo, for example; how it is
that a lens in sunlight can make paper burn; how a “walking stick” got to look so much like a
twig; why the Moon seems to follow us as we walk; what prevents us from digging a hole
down to the center of the Earth; what the definition is of “down” on a spherical Earth; how it is
possible for the body to convert yesterday’s lunch into today’s muscle and sinew; or how far is
updoes the universe go on forever, or if it does not, is there any meaning to the question of
what lies on the other side? Some of these questions are pretty easy. Others, especially the last,
are mysteries to which no one even today knows the answer. They are natural questions to ask.
Every culture has posed such questions in one way or another. Almost always the proposed
answers are in the nature of “Just So Stories,” attempted explanations divorced from
experiment, or even from careful comparative observations.

Continue reading “Can We Know the Universe?” »

 


Resume Of Dr. Manmohan Singh(PM Of INDIA) Which Is Admired By The World And Considered One Of The Best Resume Available To Date.

Born on: September 26, 1932
Place of Birth: Gah (West Punjab)
Father: Gurmukh Singh
Mother: Amrit Kaur
Married on: September 14, 1958
Wife: Gursharan Kaur
Children: Three daughters

EDUCATION:

Stood first in BA (Hons), Economics, Panjab University, Chandigarh, 1952; stood first in MA (Economics), Panjab University, Chandigarh, 1954; Wright’s Prize for distinguished performance at St John’s College, Cambridge, 1955 and 1957; Wrenbury scholar, University of Cambridge, 1957; DPhil (Oxford), DLitt (Honoris Causa); PhD thesis on India’s export competitiveness

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WHAT ARE MULTIPLE INTELLIGENCES AND HOW TO IMPROVE THEM ?

Art Of IntelligenceSeven Intelligences:
1.Linguistic 2.Bodily-Kinesthetic 3.Musical 4.Personal 5.Logical-Mathematical 6.Naturalist 7.Spatial

Linguistic Intelligence:

Linguistic Intelligence is the capacity to use language, your native language, and perhaps other languages, to express what’s on your mind and to understand other people.

Famous examples: Bill Clinton, J.K.Rowling, Tony Robbins, Winston Churchill

Linguistic Intelligence traits:

Continue reading “Multiple Intelligences For Better IQ” »