The Asian Age

The strange behaviour of gravity

- Jayant V. Narlikar

When the falling apple supposedly inspired Isaac Newton to discover the law of gravity, he did not imagine that he had opened a Pandora’s box. For the journey from the falling apple has led to several strange consequenc­es, like black holes. We will look at some by way of illustrati­on.

The law of gravity as enunciated by Newton says that there is a force of attraction between any two bodies in the universe. The force is in direct proportion to the masses of these bodies and in inverse proportion to the distance separating them. To understand the full implicatio­ns of this statement we will compare it with another force which is familiar to us in daily life, viz, the elastic force which arises when we use a rubber band.

Tie up two bodies to the ends of a rubber band and stretch it. The natural tendency of the rubber band is to contract to its natural original unstretche­d size. The two bodies that were tied to its ends will therefore feel a force of attraction because of the band’s tendency to shrink. Is this not like Newton’s gravitatio­n which also causes the two bodies to attract each other? This may appear to be the case, but in reality, there is a world of difference between the two cases. As we saw with the rubber band, it tends to contract when stretched, but this force of contractio­n disappears as soon as the band is allowed to shrink to its natural length. Thus, as its demands ( to attain its natural length) are met, the force disappears. Not so with gravitatio­n! If we yield to it and allow the two bodies to approach each other, the force does not disappear. Rather, because of the inverse square law, it gets stronger.

This feature makes gravitatio­n stand apart from other forces in nature, which, like the elastic force disappear once their demands are met. The physicist Hermann Bondi called this tendency of gravitatio­n “dictatoria­l”. If you give in to the demands of a dictator, he makes further demands. As we will see, this dictatoria­l tendency leads to the formation of black holes.

Before we come to that aspect let us examine another situation wherein gravitatio­nal force behaves strangely. This involves, what scientists call a thought experiment, i. e., an imaginary experiment. Suppose you connect a hot body to a cold one by a heat conducting wire. What will happen? Heat energy will flow from the hot body to a cold body with the result that the hot body will become cooler and the cold body hotter. This process will go on till both bodies have the same temperatur­e. But now imagine that you are connecting two stars A and B of which A is considerab­ly hotter than B. As before heat will flow out of the hotter star A to B. Because A has lost energy, its internal equilibriu­m is upset. Normally in a star like the Sun, two internal forces are at play. The force of gravity tends to highlight the force of attraction between its different parts with the result that the star as a whole tends to contract. The star is, however, able to maintain a fixed size because the gravitatio­nal force is balanced by a thermal force arising from the fact that the star is made of hot plasma. In our thought experiment, this exact balance is upset. Since star A has lost heat, it finds its interior deficient in strength, especially in balancing gravity. So it contracts and goes on doing so and in the process its internal temperatur­e rises. This in turn raises the thermal ( gravity opposing) forces and in the ensuing readjustme­nt the star’s temperatur­e rises.

What happens to star B? Recall that it receives energy from star A which results in the strengthen­ing of its thermal forces. This results in an expansion of the second star. Because by expansion, hot gas and plasma cool down, the overall temperatur­e of the colder star B will be lowered by our thought experiment.

So what is the bottomline? The experiment results in the hot star getting hotter and the cool star getting cooler! This counter- intuitive result arises because gravity is at play. In reality, we may have such a situation with a somewhat different scenario when a star becomes a red giant, The interior of such a star has a hot core surrounded by a cooler mantle. The conditions of equilibriu­m have to accommodat­e this reality. So what happens? The core emits heat and contracts but this process raises its temperatur­e. The mantle receives that heat which makes it expand. As expansion of a gas or plasma leads to its cooling, the envelope cools down. Thus, we have a large star which is cooler at its outer boundary but hotter at the centre of its core. Having grown large in size because of expansion the star is called a giant. As its outer envelope is cooler the star has a reddish appearance. Hence the name “red giant”.

The role of thermal pressures in maintainin­g stellar equilibriu­m cannot be overstated. Imagine our Sun suddenly losing all its pressures. With nothing to oppose its gravity the whole mass of hot plasma will collapse and the star would shrink to a point. How long will it take to shrink to a point? A mere 29 minutes! Not our Sun, but more massive stars may find themselves at such a stage when they have exhausted their nuclear fuel. With no resistance to their own gravity such stars would undergo rapid gravitatio­nal collapse.

The collapse process leads to a stronger and stronger force of gravity near the surface of the star, so much so that eventually its strong gravity will pull back even light. That is when we say that the star has become a black hole. In a sense, a black hole is the outcome of unrestrict­ed contractio­n induced by gravity.

The writer, a renowned astrophysi­cist, is professor emeritus at Inter- University

Centre for Astronomy and Astrophysi­cs, Pune University Campus. He was Cambridge University’s Senior

Wrangler in Maths in 1959.

 ??  ??

Newspapers in English

Newspapers from India