Dark Matter: A Cosmic Ghost Story [Around the Globe]

نویسندگان

چکیده

There is a ghost in the universe. Many things are “invisible” because they do not emit light at wavelengths we can see: newborn stars glowing infrared, microwaves from start of universe, and rapidly spinning neutron all shine, just it parts spectrum that human eyes blind to. But these still light, kind. We could call this “type one” invisibility: invisible point view beings but perfectly visible if you “see” with or microwave, radio wave eyes. over last few decades, astronomers have become aware there something truly haunting spaces our cosmos. Dark matter so invisible, got glimpse it—at all—and only guess its existence see effects has on normal surrounds it. As far as tell, dark kind two” completely across entire electromagnetic spectrum.

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Dark Matter Halos around Galaxies

We present evidence that all galaxies, of any Hubble type and luminosity, bear the kinematical signature of a mass component distributed differently from the luminous matter. We review and/or derive the DM halo properties of galaxies of different morphologies: spirals, LSBs, ellipticals, dwarf irregulars and dwarf spheroidals. We show that the halo density profile Mh(x) = Mh(1) (1 + a ) x3 x2 +...

متن کامل

Duality, dark matter and the cosmic clock

How do we know that the CMB photons originate in the early universe? We discuss the possibility of their origin from mirror neutrino annihilation and suggest an experimental test of this hypothesis. This essay was not written for any competition on the subject of gravity. Despite its remarkable success, it should be noted that the standard ΛCDM cosmology is largely an empirical affair, with no ...

متن کامل

Inhomogeneous baryogenesis , cosmic antimatter , and dark matter

A model of inhomogeneous baryogenesis based on the Affleck and Dine mechanism is described. A simple coupling of the scalar baryon field to the inflaton allows for formation of astronomically significant bubbles with a large baryon (or antibaryon) asymmetry. During the farther evolution these domains form compact stellar-like objects, or lower density clouds, or primordial black holes of differ...

متن کامل

Dark matter production from cosmic necklaces

Cosmic strings have gained a great interest, since they are formed in a large class of brane inflationary models. The most interesting story is that cosmic strings in brane models are distinguished in future cosmological observations. If the strings in brane models are branes or superstrings that can move along compactified space, and also if there are degenerated vacua along the compactified s...

متن کامل

Cosmic strings with interacting hot dark matter

We compute the linear power spectrum of cosmic string sedeed fluctuations in the context of neutrinos with a strong self-interaction and show that it is very similar to that obtained in the context of ‘normal’ neutrinos. We compare our results with observational data and show that for any value of the cosmological parameters h and Ω0 the interacting hot dark matter power spectrum requires a lar...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: IEEE Microwave Magazine

سال: 2023

ISSN: ['1527-3342', '1557-9581']

DOI: https://doi.org/10.1109/mmm.2023.3265520