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Unanswered Questions. We have seen in this chapter that theoretical models make numerous predictions about the nature of black holes but leave many questions unanswered. Briefly describe one important but unanswered question related to black holes. If you think it will be possible to answer that question in the future, describe how we would find an answer, being as specific as possible about the evidence necessary to answer the question. If you think the question will never be answered, explain why you think it is impossible to answer.

Short Answer

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The information paradox questions whether information is lost in black holes; resolving it may require detecting and analyzing Hawking radiation.

Step by step solution

01

Identify an Unanswered Question

One significant unanswered question in the study of black holes is the information paradox, which asks: What happens to the information about matter that falls into a black hole? According to general relativity, this information is lost forever as the matter falls past the event horizon. However, this idea conflicts with quantum mechanics, which states that information must be preserved.
02

Assess Possibility of Finding an Answer

It is possible that this question could be answered in the future. One potential way to resolve the black hole information paradox is through a more comprehensive understanding of quantum gravity. Currently, physicists are exploring theories such as string theory and loop quantum gravity, which could reconcile quantum mechanics and general relativity.
03

Outline Specific Evidence Needed

Evidence needed to answer this question includes the detection and analysis of Hawking radiation, a theoretical form of radiation that could carry information away from a black hole. If Hawking radiation is observed to carry information, it would support the theory that information is not lost in black holes, thus resolving the paradox.
04

Discuss Challenges and Future Prospects

Detecting Hawking radiation is extremely challenging due to its weak nature and the immense distances involved. Advanced technologies and more sensitive equipment may be required to observe and analyze this radiation in the future.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

The Information Paradox
Black holes present one of the most intriguing puzzles in physics: the information paradox. When matter falls into a black hole, classical physics, described by general relativity, suggests that all the information about that matter is lost forever beyond the event horizon. On the other hand, quantum mechanics insists that information cannot be destroyed. This conflict between two fundamental theories poses a major unanswered question: if information is not destroyed, what happens to it? This paradox challenges our understanding of the universe, balancing on the edge of gravity and quantum mechanics.

To potentially resolve this paradox, physicists are considering theories that might meld quantum mechanics with gravitational forces, such as string theory or loop quantum gravity. These theories suggest that the fabric of space-time itself could hold the key to preserving information. However, the pursuit of these theories remains in its early stages, and conclusive evidence has yet to be gathered. An answer to this paradox is not only achievable but could revolutionize the way we understand black holes and the universe as a whole.
Quantum Gravity
Quantum gravity seeks to unify two crucial pillars of physics: quantum mechanics, which describes the microscopic world of particles, and general relativity, which explains the macroscopic world of gravity and cosmic scales. The quest for a theory of quantum gravity aims to reconcile these two frameworks into a single, coherent theory that can describe phenomena where both quantum effects and gravitational forces are significant, such as inside black holes or the beginning of the universe.

Current approaches to quantum gravity include:
  • **String Theory**: Suggests that the fundamental constituents of the universe are not point-like particles but instead tiny vibrating strings. These strings can manifest as different particles, including the graviton, which is theorized to mediate gravity.
  • **Loop Quantum Gravity**: Proposes that space-time itself has a discrete structure at the smallest scales, composed of loops connected in a lattice-like network.
Yet, both theories are incomplete and require experimental verification. Understanding quantum gravity not only promises to clarify the information paradox but also enhance our overall understanding of the universe, opening doors to new technologies and insights.
Hawking Radiation
Hawking radiation is a theoretical concept first introduced by physicist Stephen Hawking, proposing that black holes are not entirely black but emit small amounts of thermal radiation, now known as Hawking radiation. This was a groundbreaking suggestion because it challenged the idea that nothing could escape a black hole.

Here's how it might work: Near a black hole's event horizon, particle-antiparticle pairs can spontaneously form. Sometimes these pairs are split, with one particle escaping, being observed as Hawking radiation, while the other falls into the black hole. This process seems to allow for energy—or even information—to leak from the black hole.

Detecting Hawking radiation would require extremely sensitive instruments due to its faint nature. The radiation provides a potential mechanism for resolving the information paradox by possibly being the medium through which information escapes a black hole. Although direct observation remains elusive, advancements in astrophysical instrumentation might one day confirm the existence of Hawking radiation, therefore integrating the resolution of the information paradox into our physics framework.

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Most popular questions from this chapter

Choose the best answer to each of the following. Explain your reasoning with one or more complete sentences. What would happen if the Sun suddenly became a black hole without changing its mass? (a) The black hole would quickly suck in Earth. (b) Earth would gradually spiral into the black hole. (c) Earth would remain in the same orbit.

Why do we think that supernovae should sometimes form black holes? What observational evidence supports the existence of black holes?

Be sure to show all calculations clearly and state your final answers in complete sentences. Neutron Star Density. A typical neutron star has a mass of about \(1.5 M_{\text {Sun }}\) and a radius of 10 kilometers. a. Calculate the average density of a neutron star, in kilograms per cubic centimeter. b. Compare the mass of \(1 \mathrm{cm}^{3}\) of neutron star material to the mass of Mount Everest \(\left(=5 \times 10^{10} \mathrm{kg}\right)\).

Be sure to show all calculations clearly and state your final answers in complete sentences. A Black Hole II? You've just discovered another new X-ray binary, which we will call Hyp-X2 ("Hyp" for hypothetical). The system Hyp-X2 contains a bright, G2 main-sequence star orbiting an unseen companion. The separation of the stars is estimated to be 12 million kilometers, and the orbital period of the visible star is 5 days. a. Use Newton's version of Kepler's third law to calculate the sum of the masses of the two stars in the system. (Hint: See Mathematical Insight \(15.4 .\) ) Give your answer in both kilograms and solar masses \(\left(M_{\mathrm{Sun}}=2.0 \times 10^{30} \mathrm{kg}\right)\) b. Determine the mass of the unseen companion. Is it a neutron star or a black hole? Explain. (Hint: A G2 mainsequence star has a mass of \(1 M\) sun.)

In what sense is a black hole like a hole in the observable universe? Define the event horizon and the Schwarzschild radius, and describe the three basic properties of a black hole.

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