Example of Physics of the Dark Universe format
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Example of Physics of the Dark Universe format Example of Physics of the Dark Universe format Example of Physics of the Dark Universe format Example of Physics of the Dark Universe format Example of Physics of the Dark Universe format Example of Physics of the Dark Universe format Example of Physics of the Dark Universe format Example of Physics of the Dark Universe format Example of Physics of the Dark Universe format Example of Physics of the Dark Universe format Example of Physics of the Dark Universe format Example of Physics of the Dark Universe format Example of Physics of the Dark Universe format Example of Physics of the Dark Universe format Example of Physics of the Dark Universe format Example of Physics of the Dark Universe format Example of Physics of the Dark Universe format
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Physics of the Dark Universe — Template for authors

Publisher: Elsevier
Categories Rank Trend in last 3 yrs
Space and Planetary Science #21 of 97 down down by 10 ranks
Astronomy and Astrophysics #22 of 88 down down by 10 ranks
journal-quality-icon Journal quality:
High
calendar-icon Last 4 years overview: 373 Published Papers | 2521 Citations
indexed-in-icon Indexed in: Scopus
last-updated-icon Last updated: 03/07/2020
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Related Journals

open access Open Access

Oxford University Press

Quality:  
High
CiteRatio: 9.2
SJR: 2.067
SNIP: 0.962
open access Open Access

Elsevier

Quality:  
High
CiteRatio: 4.1
SJR: 1.099
SNIP: 1.093
open access Open Access

Elsevier

Quality:  
High
CiteRatio: 4.6
SJR: 0.682
SNIP: 1.274
open access Open Access

Elsevier

Quality:  
High
CiteRatio: 7.7
SJR: 1.785
SNIP: 1.24

Journal Performance & Insights

CiteRatio

SCImago Journal Rank (SJR)

Source Normalized Impact per Paper (SNIP)

A measure of average citations received per peer-reviewed paper published in the journal.

Measures weighted citations received by the journal. Citation weighting depends on the categories and prestige of the citing journal.

Measures actual citations received relative to citations expected for the journal's category.

6.8

20% from 2019

CiteRatio for Physics of the Dark Universe from 2016 - 2020
Year Value
2020 6.8
2019 8.5
2018 8.6
2017 8.7
2016 10.1
graph view Graph view
table view Table view

1.485

2% from 2019

SJR for Physics of the Dark Universe from 2016 - 2020
Year Value
2020 1.485
2019 1.459
2018 2.239
2017 2.475
2016 3.26
graph view Graph view
table view Table view

1.164

19% from 2019

SNIP for Physics of the Dark Universe from 2016 - 2020
Year Value
2020 1.164
2019 0.981
2018 1.297
2017 1.469
2016 1.991
graph view Graph view
table view Table view

insights Insights

  • CiteRatio of this journal has decreased by 20% in last years.
  • This journal’s CiteRatio is in the top 10 percentile category.

insights Insights

  • SJR of this journal has increased by 2% in last years.
  • This journal’s SJR is in the top 10 percentile category.

insights Insights

  • SNIP of this journal has increased by 19% in last years.
  • This journal’s SNIP is in the top 10 percentile category.

Physics of the Dark Universe

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Elsevier

Physics of the Dark Universe

Approved by publishing and review experts on SciSpace, this template is built as per for Physics of the Dark Universe formatting guidelines as mentioned in Elsevier author instructions. The current version was created on 03 Jul 2020 and has been used by 752 authors to write and format their manuscripts to this journal.

Space and Planetary Science

Astronomy and Astrophysics

Earth and Planetary Sciences

i
Last updated on
03 Jul 2020
i
ISSN
2212-6864
i
Impact Factor
Very High - 3.181
i
Open Access
No
i
Sherpa RoMEO Archiving Policy
Green faq
i
Plagiarism Check
Available via Turnitin
i
Endnote Style
Download Available
i
Bibliography Name
elsarticle-num
i
Citation Type
Numbered
[25]
i
Bibliography Example
G. E. Blonder, M. Tinkham, T. M. Klapwijk, Transition from metallic to tunneling regimes in superconducting microconstrictions: Excess current, charge imbalance, and supercurrent conversion, Phys. Rev. B 25 (7) (1982) 4515–4532. URL 10.1103/PhysRevB.25.4515

Top papers written in this journal

open accessOpen access Journal Article DOI: 10.1016/J.DARK.2016.10.002
The clustering of massive Primordial Black Holes as Dark Matter: measuring their mass distribution with Advanced LIGO
Sebastien Clesse1, Juan Garcia-Bellido2

Abstract:

The recent detection by Advanced LIGO of gravitational waves (GW) from the merging of a binary black hole system sets new limits on the merging rates of massive primordial black holes (PBH) that could be a significant fraction or even the totality of the dark matter in the Universe. aLIGO opens the way to the determination of... The recent detection by Advanced LIGO of gravitational waves (GW) from the merging of a binary black hole system sets new limits on the merging rates of massive primordial black holes (PBH) that could be a significant fraction or even the totality of the dark matter in the Universe. aLIGO opens the way to the determination of the distribution and clustering of such massive PBH. If PBH clusters have a similar density to the one observed in ultra-faint dwarf galaxies, we find merging rates comparable to aLIGO expectations. Massive PBH dark matter predicts the existence of thousands of those dwarf galaxies where star formation is unlikely because of gas accretion onto PBH, which would possibly provide a solution to the missing satellite and too-big-to-fail problems. Finally, we study the possibility of using aLIGO and future GW antennas to measure the abundance and mass distribution of PBH in the range [5–200] M ⊙ to 10% accuracy. read more read less

Topics:

Primordial black hole (59%)59% related to the paper, Binary black hole (58%)58% related to the paper, Dark matter (55%)55% related to the paper, LIGO (54%)54% related to the paper, Galaxy (53%)53% related to the paper
429 Citations
open accessOpen access Journal Article DOI: 10.1016/J.DARK.2015.12.005
The characterization of the gamma-ray signal from the central Milky Way: A case for annihilating dark matter

Abstract:

Past studies have identified a spatially extended excess of ∼1–3 GeV gamma rays from the region surrounding the Galactic Center, consistent with the emission expected from annihilating dark matter. We revisit and scrutinize this signal with the intention of further constraining its characteristics and origin. By applying cuts... Past studies have identified a spatially extended excess of ∼1–3 GeV gamma rays from the region surrounding the Galactic Center, consistent with the emission expected from annihilating dark matter. We revisit and scrutinize this signal with the intention of further constraining its characteristics and origin. By applying cuts to the Fermi event parameter CTBCORE, we suppress the tails of the point spread function and generate high resolution gamma-ray maps, enabling us to more easily separate the various gamma-ray components. Within these maps, we find the GeV excess to be robust and highly statistically significant, with a spectrum, angular distribution, and overall normalization that is in good agreement with that predicted by simple annihilating dark matter models. For example, the signal is very well fit by a 36–51 GeV dark matter particle annihilating to b b with an annihilation cross section of σ v = ( 1 − 3 ) × 1 0 − 26 cm 3 / s (normalized to a local dark matter density of 0.4 GeV / cm 3 ). Furthermore, we confirm that the angular distribution of the excess is approximately spherically symmetric and centered around the dynamical center of the Milky Way (within ∼ 0.0 5 ∘ of Sgr A ∗ ), showing no sign of elongation along the Galactic Plane. The signal is observed to extend to at least ≃ 1 0 ∘ from the Galactic Center, which together with its other morphological traits disfavors the possibility that this emission originates from previously known or modeled pulsar populations. read more read less

Topics:

Dark matter (59%)59% related to the paper, Galactic plane (57%)57% related to the paper, Galaxy (56%)56% related to the paper, Galactic Center (54%)54% related to the paper, Milky Way (54%)54% related to the paper
View PDF
426 Citations
open accessOpen access Journal Article DOI: 10.1016/J.DARK.2015.08.001
Simplified Models for Dark Matter Searches at the LHC
Jalal Abdallah1, Henrique Araujo2, Alexandre Arbey3, Alexandre Arbey4, Alexandre Arbey5, Adi Ashkenazi6, Alexander Belyaev7, Joshua Berger8, Celine Boehm9, Antonio Boveia3, Amelia Jean Brennan10, James John Brooke, Oliver Buchmueller2, Matthew R. Buckley11, Giorgio Busoni12, Lorenzo Calibbi13, Lorenzo Calibbi14, Sushil Chauhan15, Nadir Daci16, Gavin Davies2, Isabelle De Bruyn16, Paul De Jong, Albert De Roeck3, Kees de Vries2, D. Del Re, Andrea De Simone12, Andrea Di Simone17, Caterina Doglioni18, Matthew J. Dolan8, Herbi K. Dreiner19, John Ellis3, John Ellis20, Sarah Catherine Eno21, Erez Etzion6, Malcolm Fairbairn20, Brian Feldstein22, Henning Flaecher, Eric Feng23, Patrick J. Fox24, Marie-Helene Genest25, Loukas Gouskos26, Johanna Gramling18, Ulrich Haisch22, Ulrich Haisch3, Roni Harnik24, Anthony Hibbs22, Siewyan Hoh27, W. Hopkins28, Valerio Ippolito29, Thomas Jacques18, Felix Kahlhoefer, Valentin V. Khoze9, Russell Kirk30, Andreas Korn31, Khristian Kotov32, Shuichi Kunori33, Greg Landsberg34, Sebastian Liem35, Tongyan Lin36, Steven Lowette16, Robyn Lucas2, Robyn Lucas37, Luca Malgeri3, Sarah Malik2, Christopher McCabe35, Christopher McCabe9, Alaettin Serhan Mete38, Enrico Morgante18, Stephen Mrenna24, Yu Nakahama39, Yu Nakahama3, Dave M Newbold, Karl Nordström40, Priscilla Pani, Michele Papucci41, Michele Papucci42, Sophio Pataraia, Bjoern Penning36, Deborah Pinna43, Giacomo Polesello, Davide Racco18, Emanuele Re22, Antonio Riotto18, Thomas G. Rizzo8, David Salek35, Subir Sarkar22, S. Schramm44, P. Skubic45, Oren Slone6, Juri Smirnov46, Yotam Soreq47, T. J. Sumner2, Tim M. P. Tait38, Marc Thomas7, Marc Thomas37, Ian R Tomalin37, C. Tunnell, Alessandro Vichi3, Tomer Volansky6, Neal Weiner48, Stephen M. West30, Monika Wielers37, Steven Worm37, Itay Yavin49, Itay Yavin50, Bryan Zaldivar14, Ning Zhou38, Kathryn M. Zurek41, Kathryn M. Zurek42

Abstract:

This document outlines a set of simplified models for dark matter and its interactions with Standard Model particles. It is intended to summarize the main characteristics that these simplified models have when applied to dark matter searches at the LHC, and to provide a number of useful expressions for reference. The list of ... This document outlines a set of simplified models for dark matter and its interactions with Standard Model particles. It is intended to summarize the main characteristics that these simplified models have when applied to dark matter searches at the LHC, and to provide a number of useful expressions for reference. The list of models includes both s-channel and t-channel scenarios. For s-channel, spin-0 and spin-1 mediation is discussed, and also realizations where the Higgs particle provides a portal between the dark and visible sectors. The guiding principles underpinning the proposed simplified models are spelled out, and some suggestions for implementation are presented. read more read less

Topics:

Dark matter (52%)52% related to the paper
View PDF
318 Citations
open accessOpen access Journal Article DOI: 10.1016/J.DARK.2013.06.003
Two emission mechanisms in the Fermi Bubbles: A possible signal of annihilating dark matter
Dan Hooper1, Dan Hooper2, Tracy R. Slatyer3

Abstract:

We study the variation of the spectrum of the Fermi Bubbles with Galactic latitude. Far from the Galactic plane ( | b | ≳ 30°), the observed gamma-ray emission is nearly invariant with latitude, and is consistent with arising from inverse Compton scattering of the interstellar radiation field by cosmic-ray electrons with an a... We study the variation of the spectrum of the Fermi Bubbles with Galactic latitude. Far from the Galactic plane ( | b | ≳ 30°), the observed gamma-ray emission is nearly invariant with latitude, and is consistent with arising from inverse Compton scattering of the interstellar radiation field by cosmic-ray electrons with an approximately power-law spectrum. The same electrons in the presence of microgauss-scale magnetic fields can also generate the the observed microwave “haze”. At lower latitudes ( | b | ≲ 20°), in contrast, the spectrum of the emission correlated with the Bubbles possesses a pronounced spectral feature peaking at ∼1–4 GeV (in E2dN/dE) which cannot be generated by any realistic spectrum of electrons. Instead, we conclude that a second (non-inverse-Compton) emission mechanism must be responsible for the bulk of the low-energy, low-latitude emission. This second component is spectrally similar to the excess GeV emission previously reported from the Galactic Center (GC), and also appears spatially consistent with a luminosity per volume falling approximately as r−2.4, where r is the distance from the GC. Consequently, we argue that the spectral feature visible in the low-latitude Bubbles is most likely the extended counterpart of the GC excess, now detected out to at least ∼2–3 kpc from the GC. The spectrum and angular distribution of the signal is broadly consistent with that predicted from ∼10 GeV dark matter particles annihilating to leptons, or from ∼50 GeV dark matter particles annihilating to quarks, following a distribution similar to, but slightly steeper than, the canonical Navarro–Frenk–White (NFW) profile. We also consider millisecond pulsars as a possible astrophysical explanation for the signal, as observed millisecond pulsars possess a spectral cutoff at approximately the required energy. Any such scenario would require a large population of unresolved millisecond pulsars extending at least 2–3 kpc from the GC. read more read less

Topics:

Emission spectrum (58%)58% related to the paper, Millisecond pulsar (57%)57% related to the paper, Dark matter (55%)55% related to the paper, Fermi Gamma-ray Space Telescope (54%)54% related to the paper, Galactic plane (54%)54% related to the paper
301 Citations
open accessOpen access Journal Article DOI: 10.1016/J.DARK.2016.02.001
Beyond ΛCDM: Problems, solutions, and the road ahead

Abstract:

Despite its continued observational successes, there is a persistent (and growing) interest in extending cosmology beyond the standard model, ΛCDM. This is motivated by a range of apparently serious theoretical issues, involving such questions as the cosmological constant problem, the particle nature of dark matter, the valid... Despite its continued observational successes, there is a persistent (and growing) interest in extending cosmology beyond the standard model, ΛCDM. This is motivated by a range of apparently serious theoretical issues, involving such questions as the cosmological constant problem, the particle nature of dark matter, the validity of general relativity on large scales, the existence of anomalies in the CMB and on small scales, and the predictivity and testability of the inflationary paradigm. In this paper, we summarize the current status of ΛCDM as a physical theory, and review investigations into possible alternatives along a number of different lines, with a particular focus on highlighting the most promising directions. While the fundamental problems are proving reluctant to yield, the study of alternative cosmologies has led to considerable progress, with much more to come if hopes about forthcoming high-precision observations and new theoretical ideas are fulfilled. read more read less

Topics:

Cosmological constant problem (51%)51% related to the paper
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294 Citations
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3. Can I cite my article in multiple styles in Physics of the Dark Universe?

Of course! We support all the top citation styles, such as APA style, MLA style, Vancouver style, Harvard style, and Chicago style. For example, when you write your paper and hit autoformat, our system will automatically update your article as per the Physics of the Dark Universe citation style.

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Sign up for our free trial, and you'll be able to use all our features for seven days. You'll see how helpful they are and how inexpensive they are compared to other options, Especially for Physics of the Dark Universe.

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Yes. You can choose the right template, copy-paste the contents from the word document, and click on auto-format. Once you're done, you'll have a publish-ready paper Physics of the Dark Universe that you can download at the end.

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After writing your paper autoformatting in Physics of the Dark Universe, you can download it in multiple formats, viz., PDF, Docx, and LaTeX.

12. Is Physics of the Dark Universe's impact factor high enough that I should try publishing my article there?

To be honest, the answer is no. The impact factor is one of the many elements that determine the quality of a journal. Few of these factors include review board, rejection rates, frequency of inclusion in indexes, and Eigenfactor. You need to assess all these factors before you make your final call.

13. What is Sherpa RoMEO Archiving Policy for Physics of the Dark Universe?

SHERPA/RoMEO Database

We extracted this data from Sherpa Romeo to help researchers understand the access level of this journal in accordance with the Sherpa Romeo Archiving Policy for Physics of the Dark Universe. The table below indicates the level of access a journal has as per Sherpa Romeo's archiving policy.

RoMEO Colour Archiving policy
Green Can archive pre-print and post-print or publisher's version/PDF
Blue Can archive post-print (ie final draft post-refereeing) or publisher's version/PDF
Yellow Can archive pre-print (ie pre-refereeing)
White Archiving not formally supported
FYI:
  1. Pre-prints as being the version of the paper before peer review and
  2. Post-prints as being the version of the paper after peer-review, with revisions having been made.

14. What are the most common citation types In Physics of the Dark Universe?

The 5 most common citation types in order of usage for Physics of the Dark Universe are:.

S. No. Citation Style Type
1. Author Year
2. Numbered
3. Numbered (Superscripted)
4. Author Year (Cited Pages)
5. Footnote

15. How do I submit my article to the Physics of the Dark Universe?

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Yes, SciSpace provides this functionality. After signing up, you would need to import your existing references from Word or Bib file to SciSpace. Then SciSpace would allow you to download your references in Physics of the Dark Universe Endnote style according to Elsevier guidelines.

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