joseph

Skip navigationDepartment of PhysicsSearchUW Home

http://images.physics-edu.org/trans.gif

http://images.physics-edu.org/trans.gif

http://images.physics-edu.org/trans.gif

The main points discussed in the book "Structure of Atom"     Acceptance of the New Physics           

 

http://images.physics-edu.org/corner1.gifhttp://images.physics-edu.org/corner-rt.gif
http://images.physics-edu.org/corner-left.gif

 

UW Home Page

 Structure of Atom Amazon Kindle Ebook

 

BASIC PHYSICS

Structure of atom

 

Structure of electron

 

What is light?

 

How is nuclear energy released?

 

Space matter or Aether


IN DEPTH

How is light emitted?

 

Line spectrum of hydrogen atom

 

How radio waves are prduced?

 

How is chemical energy released?

 

Wave nature of matter

 

Electric field and magnetic field

 

Pair production of electron and positron

 

Some important phenomena in the atomic world

 

Star light bending

 

Reference

 

Researcher and author

 

Contact


 

http://images.physics-edu.org/trans.gif

 

Zeeman effect, Paschen-Back effect & Stark effect

   The electron configuration in a multi electron atom is determined by three factors. a) Attractive force from the nucleus, b) repulsive forces between electrons, and c) buoyant force exerted by space matter. When an atom is placed in a strong- electric field or magnetic field, its electron configuration is shifted from the atom’s normal state. That is, some of the electrons in the atom (mostly electrons in the outer regions) are shifted from their electron shells to inner or outer transitory shells, by the influence of the external field. When  such   an  atom  is  excited,  the atom can emit radiations in the natural frequencies of the transitory shells, to which the electrons are shifted, as well as in the natural frequencies of the electrons shells, which are not affected by the applied field. The effects are the direct indications for the strengths of the fields. I.e. when a weak field can affect only outer electrons, a strong field can influence both the inner  and  outer     electrons   alike.   Lighter elements can demonstrate the effects in a weaker field comparatively than heavy elements, because of the binding force on the electrons in a lighter element is much less than that of heavy elements.

 

Absorption spectrum

    When a cooled gas is placed in the path of a continues spectrum of light, dark absorption lines will be appeared in the resulting spectrum. Each shell (electron shells and transitory shells)  of  an  atom  has  its own unique natural frequency or resonant frequency. When a  photon  falls  on  an electron and the photon’s frequency matches with the natural frequency of the shell (electron shell or transitory shell) in which the electron exist at that moment, the    photon    will    be  absorbed by the electron. This absorption causes, the photon that absorbed by the atom,   will   be    absent    in   the resulting spectrum. This is the reason for the absorption spectrum. Considering hydrogen atom, absorption lines cannot be detected in the case of cold hydrogen gas by continuous spectra of light of less than 3 electron volt (red to blue light photons, but not in the ultraviolet). In this case, absorption lines become only measurable when the electron resides temporarily in the corresponding transitory shell for which the natural frequencies of oscillations correspond to the Balmer, Pashen, Brackett, and Pfund series.

 

Structure of atom  What is light? How is nuclear energy released? Space matter or Aether . . . . . . . . . . . . . . . . . . . . . .

 

 

 

 

 

                                      © http://physics-edu.org Author