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Heisenberg's uncertainty principle quantifies the inability to precisely locate the particle given its conjugate momentum. According to one interpretation, as the result of a measurement, the wave function containing the probability information for a system collapses from a given initial state to a particular eigenstate. The probability distribution of an observable in a given state can be found by computing the spectral decomposition of the corresponding operator. Heisenberg's uncertainty principle is represented by the statement that the operators corresponding to certain observables do not commute.

The probabilistic nature of quantum mechanics thus stems from the act of measurement. This is one of the most difficult aspects of quantum systems to understand. It was the central topic in the famous Bohr—Einstein debates , in which the two scientists attempted to clarify these fundamental principles by way of thought experiments. In the decades after the formulation of quantum mechanics, the question of what constitutes a "measurement" has been extensively studied.

Newer interpretations of quantum mechanics have been formulated that do away with the concept of " wave function collapse " see, for example, the relative state interpretation. The basic idea is that when a quantum system interacts with a measuring apparatus, their respective wave functions become entangled , so that the original quantum system ceases to exist as an independent entity.

For details, see the article on measurement in quantum mechanics. Generally, quantum mechanics does not assign definite values. Instead, it makes a prediction using a probability distribution ; that is, it describes the probability of obtaining the possible outcomes from measuring an observable. Often these results are skewed by many causes, such as dense probability clouds. Probability clouds are approximate but better than the Bohr model whereby electron location is given by a probability function , the wave function eigenvalue , such that the probability is the squared modulus of the complex amplitude , or quantum state nuclear attraction.

Hence, uncertainty is involved in the value. There are, however, certain states that are associated with a definite value of a particular observable. These are known as eigenstates of the observable "eigen" can be translated from German as meaning "inherent" or "characteristic". In the everyday world, it is natural and intuitive to think of everything every observable as being in an eigenstate. Everything appears to have a definite position, a definite momentum, a definite energy, and a definite time of occurrence.

However, quantum mechanics does not pinpoint the exact values of a particle's position and momentum since they are conjugate pairs or its energy and time since they too are conjugate pairs. Rather, it provides only a range of probabilities in which that particle might be given its momentum and momentum probability. Therefore, it is helpful to use different words to describe states having uncertain values and states having definite values eigenstates. Usually, a system will not be in an eigenstate of the observable particle we are interested in.

However, if one measures the observable, the wave function will instantaneously be an eigenstate or "generalized" eigenstate of that observable. This process is known as wave function collapse , a controversial and much-debated process [33] that involves expanding the system under study to include the measurement device. If one knows the corresponding wave function at the instant before the measurement, one will be able to compute the probability of the wave function collapsing into each of the possible eigenstates.

For example, the free particle in the previous example will usually have a wave function that is a wave packet centered around some mean position x 0 neither an eigenstate of position nor of momentum. When one measures the position of the particle, it is impossible to predict with certainty the result.

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After the measurement is performed, having obtained some result x , the wave function collapses into a position eigenstate centered at x. During a measurement , on the other hand, the change of the initial wave function into another, later wave function is not deterministic, it is unpredictable i. A time-evolution simulation can be seen here. Wave functions change as time progresses. However, the wave packet will also spread out as time progresses, which means that the position becomes more uncertain with time. This also has the effect of turning a position eigenstate which can be thought of as an infinitely sharp wave packet into a broadened wave packet that no longer represents a definite, certain position eigenstate.

Many systems that are treated dynamically in classical mechanics are described by such "static" wave functions. For example, a single electron in an unexcited atom is pictured classically as a particle moving in a circular trajectory around the atomic nucleus , whereas in quantum mechanics, it is described by a static, spherically symmetric wave function surrounding the nucleus Fig.

Whereas the absolute value of the probability amplitude encodes information about probabilities, its phase encodes information about the interference between quantum states. This gives rise to the "wave-like" behavior of quantum states. There exist several techniques for generating approximate solutions, however. In the important method known as perturbation theory , one uses the analytic result for a simple quantum mechanical model to generate a result for a more complicated model that is related to the simpler model by for one example the addition of a weak potential energy.

Another method is the "semi-classical equation of motion" approach, which applies to systems for which quantum mechanics produces only weak small deviations from classical behavior.

Where is it, the foundation of quantum reality?

These deviations can then be computed based on the classical motion. This approach is particularly important in the field of quantum chaos. There are numerous mathematically equivalent formulations of quantum mechanics. Especially since Werner Heisenberg was awarded the Nobel Prize in Physics in for the creation of quantum mechanics, the role of Max Born in the development of QM was overlooked until the Nobel award. The role is noted in a biography of Born, which recounts his role in the matrix formulation of quantum mechanics, and the use of probability amplitudes.

Heisenberg himself acknowledges having learned matrices from Born, as published in a festschrift honoring Max Planck. Examples of observables include energy , position , momentum , and angular momentum. Observables can be either continuous e. This is the quantum-mechanical counterpart of the action principle in classical mechanics.

The rules of quantum mechanics are fundamental. These can be chosen appropriately in order to obtain a quantitative description of a quantum system. An important guide for making these choices is the correspondence principle , which states that the predictions of quantum mechanics reduce to those of classical mechanics when a system moves to higher energies or, equivalently, larger quantum numbers, i. In other words, classical mechanics is simply a quantum mechanics of large systems. This "high energy" limit is known as the classical or correspondence limit.

One can even start from an established classical model of a particular system, then attempt to guess the underlying quantum model that would give rise to the classical model in the correspondence limit. When quantum mechanics was originally formulated, it was applied to models whose correspondence limit was non-relativistic classical mechanics.

For instance, the well-known model of the quantum harmonic oscillator uses an explicitly non-relativistic expression for the kinetic energy of the oscillator, and is thus a quantum version of the classical harmonic oscillator. While these theories were successful in explaining many experimental results, they had certain unsatisfactory qualities stemming from their neglect of the relativistic creation and annihilation of particles. A fully relativistic quantum theory required the development of quantum field theory , which applies quantization to a field rather than a fixed set of particles.

The first complete quantum field theory, quantum electrodynamics , provides a fully quantum description of the electromagnetic interaction. The full apparatus of quantum field theory is often unnecessary for describing electrodynamic systems.

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A simpler approach, one that has been employed since the inception of quantum mechanics, is to treat charged particles as quantum mechanical objects being acted on by a classical electromagnetic field. This "semi-classical" approach fails if quantum fluctuations in the electromagnetic field play an important role, such as in the emission of photons by charged particles. Quantum field theories for the strong nuclear force and the weak nuclear force have also been developed. The quantum field theory of the strong nuclear force is called quantum chromodynamics , and describes the interactions of subnuclear particles such as quarks and gluons.

The weak nuclear force and the electromagnetic force were unified, in their quantized forms, into a single quantum field theory known as electroweak theory , by the physicists Abdus Salam , Sheldon Glashow and Steven Weinberg. These three men shared the Nobel Prize in Physics in for this work. It has proven difficult to construct quantum models of gravity , the remaining fundamental force. Semi-classical approximations are workable, and have led to predictions such as Hawking radiation.

However, the formulation of a complete theory of quantum gravity is hindered by apparent incompatibilities between general relativity the most accurate theory of gravity currently known and some of the fundamental assumptions of quantum theory. The resolution of these incompatibilities is an area of active research, and theories such as string theory are among the possible candidates for a future theory of quantum gravity. Classical mechanics has also been extended into the complex domain , with complex classical mechanics exhibiting behaviors similar to quantum mechanics.

Predictions of quantum mechanics have been verified experimentally to an extremely high degree of accuracy. For microscopic bodies, the extension of the system is much smaller than the coherence length , which gives rise to long-range entanglement and other nonlocal phenomena characteristic of quantum systems.

A big difference between classical and quantum mechanics is that they use very different kinematic descriptions. In Niels Bohr 's mature view, quantum mechanical phenomena are required to be experiments, with complete descriptions of all the devices for the system, preparative, intermediary, and finally measuring. The descriptions are in macroscopic terms, expressed in ordinary language, supplemented with the concepts of classical mechanics. Quantum mechanics does not admit a completely precise description, in terms of both position and momentum, of an initial condition or "state" in the classical sense of the word that would support a precisely deterministic and causal prediction of a final condition.

For a stationary process, the initial and final condition are the same. For a transition, they are different. Obviously by definition, if only the initial condition is given, the process is not determined. For many experiments, it is possible to think of the initial and final conditions of the system as being a particle. In some cases it appears that there are potentially several spatially distinct pathways or trajectories by which a particle might pass from initial to final condition. It is an important feature of the quantum kinematic description that it does not permit a unique definite statement of which of those pathways is actually followed.

Only the initial and final conditions are definite, and, as stated in the foregoing paragraph, they are defined only as precisely as allowed by the configuration space description or its equivalent. In every case for which a quantum kinematic description is needed, there is always a compelling reason for this restriction of kinematic precision. An example of such a reason is that for a particle to be experimentally found in a definite position, it must be held motionless; for it to be experimentally found to have a definite momentum, it must have free motion; these two are logically incompatible.

Classical kinematics does not primarily demand experimental description of its phenomena. It allows completely precise description of an instantaneous state by a value in phase space, the Cartesian product of configuration and momentum spaces. This description simply assumes or imagines a state as a physically existing entity without concern about its experimental measurability. Such a description of an initial condition, together with Newton's laws of motion, allows a precise deterministic and causal prediction of a final condition, with a definite trajectory of passage.

Hamiltonian dynamics can be used for this. Classical kinematics also allows the description of a process analogous to the initial and final condition description used by quantum mechanics. Lagrangian mechanics applies to this. Even with the defining postulates of both Einstein's theory of general relativity and quantum theory being indisputably supported by rigorous and repeated empirical evidence , and while they do not directly contradict each other theoretically at least with regard to their primary claims , they have proven extremely difficult to incorporate into one consistent, cohesive model.

Gravity is negligible in many areas of particle physics, so that unification between general relativity and quantum mechanics is not an urgent issue in those particular applications. However, the lack of a correct theory of quantum gravity is an important issue in physical cosmology and the search by physicists for an elegant " Theory of Everything " TOE. Consequently, resolving the inconsistencies between both theories has been a major goal of 20th- and 21st-century physics.

Many prominent physicists, including Stephen Hawking , have labored for many years in the attempt to discover a theory underlying everything. This TOE would combine not only the different models of subatomic physics, but also derive the four fundamental forces of nature — the strong force , electromagnetism , the weak force , and gravity — from a single force or phenomenon. The quest to unify the fundamental forces through quantum mechanics is still ongoing.

Quantum electrodynamics or "quantum electromagnetism" , which is currently in the perturbative regime at least the most accurately tested physical theory in competition with general relativity, [69] [70] has been successfully merged with the weak nuclear force into the electroweak force and work is currently being done to merge the electroweak and strong force into the electrostrong force. Current predictions state that at around 10 14 GeV the three aforementioned forces are fused into a single unified field.

One of those searching for a coherent TOE is Edward Witten , a theoretical physicist who formulated the M-theory , which is an attempt at describing the supersymmetrical based string theory. M-theory posits that our apparent 4-dimensional spacetime is, in reality, actually an dimensional spacetime containing 10 spatial dimensions and 1 time dimension, although 7 of the spatial dimensions are — at lower energies — completely "compactified" or infinitely curved and not readily amenable to measurement or probing.

Another popular theory is Loop quantum gravity LQG , a theory first proposed by Carlo Rovelli that describes the quantum properties of gravity. It is also a theory of quantum space and quantum time , because in general relativity the geometry of spacetime is a manifestation of gravity. LQG is an attempt to merge and adapt standard quantum mechanics and standard general relativity. The main output of the theory is a physical picture of space where space is granular. The granularity is a direct consequence of the quantization.

It has the same nature of the granularity of the photons in the quantum theory of electromagnetism or the discrete levels of the energy of the atoms. But here it is space itself which is discrete. More precisely, space can be viewed as an extremely fine fabric or network "woven" of finite loops. These networks of loops are called spin networks. The evolution of a spin network over time is called a spin foam. The predicted size of this structure is the Planck length , which is approximately 1.

According to theory, there is no meaning to length shorter than this cf. Planck scale energy. Therefore, LQG predicts that not just matter, but also space itself, has an atomic structure. Since its inception, the many counter-intuitive aspects and results of quantum mechanics have provoked strong philosophical debates and many interpretations.

Even fundamental issues, such as Max Born 's basic rules concerning probability amplitudes and probability distributions , took decades to be appreciated by society and many leading scientists. Richard Feynman once said, "I think I can safely say that nobody understands quantum mechanics. According to this interpretation, the probabilistic nature of quantum mechanics is not a temporary feature which will eventually be replaced by a deterministic theory, but instead must be considered a final renunciation of the classical idea of "causality. Albert Einstein, himself one of the founders of quantum theory, did not accept some of the more philosophical or metaphysical interpretations of quantum mechanics, such as rejection of determinism and of causality.

He is famously quoted as saying, in response to this aspect, "God does not play with dice". He held that a state of nature occurs in its own right, regardless of whether or how it might be observed. In that view, he is supported by the currently accepted definition of a quantum state, which remains invariant under arbitrary choice of configuration space for its representation, that is to say, manner of observation.

He also held that underlying quantum mechanics there should be a theory that thoroughly and directly expresses the rule against action at a distance ; in other words, he insisted on the principle of locality. He considered, but rejected on theoretical grounds, a particular proposal for hidden variables to obviate the indeterminism or acausality of quantum mechanical measurement. He considered that quantum mechanics was a currently valid but not a permanently definitive theory for quantum phenomena.

He thought its future replacement would require profound conceptual advances, and would not come quickly or easily.

Quantum Mechanics - Part 1: Crash Course Physics #43

The Bohr-Einstein debates provide a vibrant critique of the Copenhagen Interpretation from an epistemological point of view. In arguing for his views, he produced a series of objections, the most famous of which has become known as the Einstein—Podolsky—Rosen paradox. John Bell showed that this EPR paradox led to experimentally testable differences between quantum mechanics and theories that rely on added hidden variables. Experiments have been performed confirming the accuracy of quantum mechanics, thereby demonstrating that quantum mechanics cannot be improved upon by addition of hidden variables.

At first these just seemed like isolated esoteric effects, but by the mids, they were being codified in the field of quantum information theory, and led to constructions with names like quantum cryptography and quantum teleportation. Entanglement, as demonstrated in Bell-type experiments, does not, however, violate causality , since no transfer of information happens. Quantum entanglement forms the basis of quantum cryptography , which is proposed for use in high-security commercial applications in banking and government. The Everett many-worlds interpretation , formulated in , holds that all the possibilities described by quantum theory simultaneously occur in a multiverse composed of mostly independent parallel universes.

Such a superposition of consistent state combinations of different systems is called an entangled state. While the multiverse is deterministic, we perceive non-deterministic behavior governed by probabilities, because we can only observe the universe i. Everett's interpretation is perfectly consistent with John Bell 's experiments and makes them intuitively understandable.

However, according to the theory of quantum decoherence , these "parallel universes" will never be accessible to us. The inaccessibility can be understood as follows: once a measurement is done, the measured system becomes entangled with both the physicist who measured it and a huge number of other particles, some of which are photons flying away at the speed of light towards the other end of the universe. In order to prove that the wave function did not collapse, one would have to bring all these particles back and measure them again, together with the system that was originally measured.


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Not only is this completely impractical, but even if one could theoretically do this, it would have to destroy any evidence that the original measurement took place including the physicist's memory. In light of these Bell tests , Cramer formulated his transactional interpretation [78] which is unique in providing a physical explanation for the Born rule.

Quantum mechanics has had enormous [80] success in explaining many of the features of our universe.

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So how can they possibly fuse? With quantum tunneling, the wave nature of protons allows them to overlap ever so slightly, like ripples merging on the surface of a pond. The protons fuse and release a single photon. Our eyes have evolved to be exquisitely sensitive to these photons. Some recent experiments have shown that we can even detect single photons, which raises an intriguing possibility: Could humans be used to test some of the weird features of quantum mechanics?

What might such an experience be like? Three years ago, when she was a graduate student at the University of Illinois at Urbana-Champaign, Holmes was part of a team led by Paul Kwiat that showed people could detect short bursts of light consisting of just three photons. In , a competing group of researchers, led by physicist Alipasha Vaziri at Rockefeller University in New York, found that humans can indeed see single photons. Seeing, though, might not accurately describe the experience. In the near future, Holmes and Vaziri expect experiments that will test what people perceive when photons are put into strange quantum states.

For example, physicists can coax a single photon into what they call a superposition, where it exists in two different places simultaneously.


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  8. Holmes and her colleagues have proposed an experiment involving two scenarios to test whether people might directly perceive a superposition of photons. But in the other scenario, a photon would be placed in a quantum superposition that would allow it to do the seemingly impossible: travel to both the right and left sides of the retina simultaneously. Would the person then sense light on both sides of the retina? If it turns out that someone participating in the experiment did indeed perceive the photon in both places simultaneously, would that mean the person herself was in a quantum state?

    When you exert pressure against the cup with your hand, the seeming solidity comes from the resistance of electrons in the cup. And the laws of quantum mechanics limit them to specific energy levels around atoms and molecules. Our sense of touch, then, arises from an exceedingly complex interaction between electrons around the molecules of our bodies and those of the objects we encounter.

    From that information, our brain creates the illusion that we possess solid bodies moving through a world filled with other solid objects. Donald Hoffman, a cognitive neuroscientist at the University of California, Irvine, believes that our senses and brain evolved to hide the true nature of reality, not to reveal it. Hoffman likens the picture our brain constructs of the world to the graphical interface on a computer screen.

    Hoffman and his graduate students have run hundreds of thousands of computer models in recent years to test his ideas. In the simulations, artificial life-forms compete for limited resources. And in every case, the organisms programmed to emphasize fitness outcompete the various ones primed for accurate perceptions. His ideas align with what some physicists believe to be a central message of quantum theory: Reality is not completely objective — we cannot separate ourselves from the world we observe.

    Hoffman fully embraces that view. When I look at that hill over there, I create that data structure.

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    Planck himself struggled for most of his life to understand the theory he helped launch, and always believed in an objective universe that exists independently of us. By Tim Folger Wednesday, October 24, For such an in-your-face sensory organ, the nose is poorly understood. As you sip your brew, ponder this: The particles of light warming your face and entering your eyes originated a million years ago in the center of the sun, around the time our not-quite-human ancestors started to use fire. The author invites readers to plunge into the physics of micro-objects and to take a fascinating tour of the world of atoms and nuclei.

    The main questions under consideration are the structure of atoms, atomic nuclei, the substance and systematics of elementary particles, the processes of the creation of atomic nuclei and the evolution of stars as well as different applied aspects of the physics of micro-objects. Series on stability, vibration, and control of systems.

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    Series A v. Berezhnoy — The quantum world of nuclear physics-World Scientific Like it? Share with your friends!