PrepTest 39, Section 4, Question 21
With the approach of the twentieth century, the classical wave theory of radiation�a widely accepted theory in physics�began to encounter obstacles. This theory held that all electromagnetic radiation�the entire spectrum from gamma and X rays to radio frequencies, including heat and light�exists in the form of waves. One fundamental assumption of wave theory was that as the length of a wave of radiation shortens, its energy increases smoothly�like a volume dial on a radio that adjusts smoothly to any setting�and that any conceivable energy value could thus occur in nature.
The major challenge to wave theory was the behavior of thermal radiation, the radiation emitted by an object due to the object's temperature, commonly called "blackbody" radiation because experiments aimed at measuring it require objects, such as black velvet or soot, with little or no reflective capability. Physicists can monitor the radiation coming from a blackbody object and be confident that they are observing its thermal radiation and not simply reflected radiation that has originated elsewhere. Employing the principles of wave theory, physicists originally predicted that blackbody objects radiated much more at short wavelengths, such as ultraviolet, than at long wavelengths. However, physicists using advanced experimental techniques near the turn of the century did not find the predicted amount of radiation at short wavelengths�in fact, they found almost none, a result that became known among wave theorists as the "ultraviolet catastrophe."
Max Planck, a classical physicist who had made important contributions to wave theory, developed a hypothesis about atomic processes taking place in a blackbody object that broke with wave theory and accounted for the observed patterns of blackbody radiation. Planck discarded the assumption of radiation's smooth energy continuum and took the then bizarre position that these atomic processes could only involve discrete energies that jump between certain units of value�like a volume dial that "clicks" between incremental settings�and he thereby obtained numbers that perfectly fit the earlier experimental result. This directly opposed wave theory's picture of atomic processes, and the physics community was at first quite critical of Planck's hypothesis, in part because he presented it without physical explanation.
Soon thereafter, however, Albert Einstein and other physicists provided theoretical justification for Planck's hypothesis. They found that upon being hit with part of the radiation spectrum, metal surfaces give off energy at values that are discontinuous. Further, they noted a threshold along the spectrum beyond which no energy is emitted by the metal. Einstein theorized, and later found evidence to confirm, that radiation is composed of particles, now called photons, which can be emitted only in discrete units and at certain wavelengths, in accordance with Planck's speculations. So in just a few years, what was considered a catastrophe generated a new vision in physics that led to theories still in place today.
With the approach of the twentieth century, the classical wave theory of radiation�a widely accepted theory in physics�began to encounter obstacles. This theory held that all electromagnetic radiation�the entire spectrum from gamma and X rays to radio frequencies, including heat and light�exists in the form of waves. One fundamental assumption of wave theory was that as the length of a wave of radiation shortens, its energy increases smoothly�like a volume dial on a radio that adjusts smoothly to any setting�and that any conceivable energy value could thus occur in nature.
The major challenge to wave theory was the behavior of thermal radiation, the radiation emitted by an object due to the object's temperature, commonly called "blackbody" radiation because experiments aimed at measuring it require objects, such as black velvet or soot, with little or no reflective capability. Physicists can monitor the radiation coming from a blackbody object and be confident that they are observing its thermal radiation and not simply reflected radiation that has originated elsewhere. Employing the principles of wave theory, physicists originally predicted that blackbody objects radiated much more at short wavelengths, such as ultraviolet, than at long wavelengths. However, physicists using advanced experimental techniques near the turn of the century did not find the predicted amount of radiation at short wavelengths�in fact, they found almost none, a result that became known among wave theorists as the "ultraviolet catastrophe."
Max Planck, a classical physicist who had made important contributions to wave theory, developed a hypothesis about atomic processes taking place in a blackbody object that broke with wave theory and accounted for the observed patterns of blackbody radiation. Planck discarded the assumption of radiation's smooth energy continuum and took the then bizarre position that these atomic processes could only involve discrete energies that jump between certain units of value�like a volume dial that "clicks" between incremental settings�and he thereby obtained numbers that perfectly fit the earlier experimental result. This directly opposed wave theory's picture of atomic processes, and the physics community was at first quite critical of Planck's hypothesis, in part because he presented it without physical explanation.
Soon thereafter, however, Albert Einstein and other physicists provided theoretical justification for Planck's hypothesis. They found that upon being hit with part of the radiation spectrum, metal surfaces give off energy at values that are discontinuous. Further, they noted a threshold along the spectrum beyond which no energy is emitted by the metal. Einstein theorized, and later found evidence to confirm, that radiation is composed of particles, now called photons, which can be emitted only in discrete units and at certain wavelengths, in accordance with Planck's speculations. So in just a few years, what was considered a catastrophe generated a new vision in physics that led to theories still in place today.
With the approach of the twentieth century, the classical wave theory of radiation�a widely accepted theory in physics�began to encounter obstacles. This theory held that all electromagnetic radiation�the entire spectrum from gamma and X rays to radio frequencies, including heat and light�exists in the form of waves. One fundamental assumption of wave theory was that as the length of a wave of radiation shortens, its energy increases smoothly�like a volume dial on a radio that adjusts smoothly to any setting�and that any conceivable energy value could thus occur in nature.
The major challenge to wave theory was the behavior of thermal radiation, the radiation emitted by an object due to the object's temperature, commonly called "blackbody" radiation because experiments aimed at measuring it require objects, such as black velvet or soot, with little or no reflective capability. Physicists can monitor the radiation coming from a blackbody object and be confident that they are observing its thermal radiation and not simply reflected radiation that has originated elsewhere. Employing the principles of wave theory, physicists originally predicted that blackbody objects radiated much more at short wavelengths, such as ultraviolet, than at long wavelengths. However, physicists using advanced experimental techniques near the turn of the century did not find the predicted amount of radiation at short wavelengths�in fact, they found almost none, a result that became known among wave theorists as the "ultraviolet catastrophe."
Max Planck, a classical physicist who had made important contributions to wave theory, developed a hypothesis about atomic processes taking place in a blackbody object that broke with wave theory and accounted for the observed patterns of blackbody radiation. Planck discarded the assumption of radiation's smooth energy continuum and took the then bizarre position that these atomic processes could only involve discrete energies that jump between certain units of value�like a volume dial that "clicks" between incremental settings�and he thereby obtained numbers that perfectly fit the earlier experimental result. This directly opposed wave theory's picture of atomic processes, and the physics community was at first quite critical of Planck's hypothesis, in part because he presented it without physical explanation.
Soon thereafter, however, Albert Einstein and other physicists provided theoretical justification for Planck's hypothesis. They found that upon being hit with part of the radiation spectrum, metal surfaces give off energy at values that are discontinuous. Further, they noted a threshold along the spectrum beyond which no energy is emitted by the metal. Einstein theorized, and later found evidence to confirm, that radiation is composed of particles, now called photons, which can be emitted only in discrete units and at certain wavelengths, in accordance with Planck's speculations. So in just a few years, what was considered a catastrophe generated a new vision in physics that led to theories still in place today.
With the approach of the twentieth century, the classical wave theory of radiation�a widely accepted theory in physics�began to encounter obstacles. This theory held that all electromagnetic radiation�the entire spectrum from gamma and X rays to radio frequencies, including heat and light�exists in the form of waves. One fundamental assumption of wave theory was that as the length of a wave of radiation shortens, its energy increases smoothly�like a volume dial on a radio that adjusts smoothly to any setting�and that any conceivable energy value could thus occur in nature.
The major challenge to wave theory was the behavior of thermal radiation, the radiation emitted by an object due to the object's temperature, commonly called "blackbody" radiation because experiments aimed at measuring it require objects, such as black velvet or soot, with little or no reflective capability. Physicists can monitor the radiation coming from a blackbody object and be confident that they are observing its thermal radiation and not simply reflected radiation that has originated elsewhere. Employing the principles of wave theory, physicists originally predicted that blackbody objects radiated much more at short wavelengths, such as ultraviolet, than at long wavelengths. However, physicists using advanced experimental techniques near the turn of the century did not find the predicted amount of radiation at short wavelengths�in fact, they found almost none, a result that became known among wave theorists as the "ultraviolet catastrophe."
Max Planck, a classical physicist who had made important contributions to wave theory, developed a hypothesis about atomic processes taking place in a blackbody object that broke with wave theory and accounted for the observed patterns of blackbody radiation. Planck discarded the assumption of radiation's smooth energy continuum and took the then bizarre position that these atomic processes could only involve discrete energies that jump between certain units of value�like a volume dial that "clicks" between incremental settings�and he thereby obtained numbers that perfectly fit the earlier experimental result. This directly opposed wave theory's picture of atomic processes, and the physics community was at first quite critical of Planck's hypothesis, in part because he presented it without physical explanation.
Soon thereafter, however, Albert Einstein and other physicists provided theoretical justification for Planck's hypothesis. They found that upon being hit with part of the radiation spectrum, metal surfaces give off energy at values that are discontinuous. Further, they noted a threshold along the spectrum beyond which no energy is emitted by the metal. Einstein theorized, and later found evidence to confirm, that radiation is composed of particles, now called photons, which can be emitted only in discrete units and at certain wavelengths, in accordance with Planck's speculations. So in just a few years, what was considered a catastrophe generated a new vision in physics that led to theories still in place today.
The passage provides information that answers each of the following questions EXCEPT:
What did Planck's hypothesis about atomic processes try to account for?
What led to the scientific community's acceptance of Planck's ideas?
Roughly when did the blackbody radiation experiments take place?
What contributions did Planck make to classical wave theory?
What type of experiment led Einstein to formulate a theory regarding the composition of radiation?
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